From fc358ce7332053945afe16ced2a271556cdccfb7 Mon Sep 17 00:00:00 2001 From: Norbert Preining Date: Tue, 4 Feb 2020 03:01:28 +0000 Subject: CTAN sync 202002040301 --- macros/latex/contrib/physconst/CHANGELOG.md | 29 +- macros/latex/contrib/physconst/README.md | 35 +- macros/latex/contrib/physconst/physconst.dtx | 11205 ++++++++++++++++++++----- macros/latex/contrib/physconst/physconst.pdf | Bin 135843 -> 208326 bytes 4 files changed, 9200 insertions(+), 2069 deletions(-) (limited to 'macros/latex/contrib/physconst') diff --git a/macros/latex/contrib/physconst/CHANGELOG.md b/macros/latex/contrib/physconst/CHANGELOG.md index 059256090c..c765c612a0 100644 --- a/macros/latex/contrib/physconst/CHANGELOG.md +++ b/macros/latex/contrib/physconst/CHANGELOG.md @@ -13,7 +13,8 @@ - added localuninstall and distuninstall targets to the makefile ### Changed - Modified the makefile to split up generation of the .sty, .dtx, and .pdf -- Modified the .cpp so that every \DeclareRobustCommand starts a new line right away +- Modified the .cpp so that every \DeclareRobustCommand starts a new line right +away - Added a newline in the middle of the title declaration (in .cpp) - Added a newline in the middle of the \DoNotIndex declaration (in .cpp) - Added dependency on imakeidx and changed the index to 2 column. @@ -31,10 +32,30 @@ - Add disribution specific readme - Add disribution specific makefile ### Changed -- Update README to have clearer build, distribute, install, and uninstall instructions. +- Update README to have clearer build, distribute, install, and uninstall +instructions. - Distribute with .dtx instead of .sty - Reordered build, install, distribute, and uninstall sections of the README - Pulled build up one level of headings in the README - fix some typos in README - - +## [1.1.0] - 2020/02/03 +### Added +- macro for Earth's mass +- macro for Jupiter's mass +- macro for Earth's radius +- macro for Jupiter's radius +- distribution specific change log +- Numeric variant of each constant for use with e.g. tikz +### Changes +- Colomb constant in SI units had an incorrect magnitude; fixed to 10^9 instead +of 10^14 +- Vacuum permeability was incorrectly a duplicate of the permittivity. +Premeability is now the correct value. +- Mass of particles in eV was being computed incorrectly. Fixed values. +- Order of magnitude of Newton's Gravity, Boltzmann, Planck, and +Stefan-Boltzmann constants were incorrect. +- Acceleration due to gravity on Earth was accidentally a copy of G instead of g +- Acceleration due to gravity on Earth had the wrong units +- Corrected formatting of README file. +- Fixed sections of macros - the individual macros were unintentionally +subsections of the Naming Conversion diff --git a/macros/latex/contrib/physconst/README.md b/macros/latex/contrib/physconst/README.md index 8a43c78f49..8727bf5e43 100644 --- a/macros/latex/contrib/physconst/README.md +++ b/macros/latex/contrib/physconst/README.md @@ -16,7 +16,8 @@ and version 1.3c or later is part of all distributions of LaTeX version 2006/05/20 or later. # Dependencies -- [`physunits` package](https://github.com/astrobit/physunits) also available at [CTAN](https://ctan.org) +- [`physunits` package](https://github.com/astrobit/physunits) also available +at [CTAN](https://ctan.org) # Build Dependencies - some LaTeX distribution. @@ -27,7 +28,8 @@ version 2006/05/20 or later. # Files ``` - makefile GNU makefile to simplify building and installation on linux + makefile GNU makefile to simplify building and installation + on linux README.md This file. CHANGELOG.md List of changes physconst.ins The installer file @@ -40,28 +42,37 @@ version 2006/05/20 or later. 1. `make` ## Otherwise -1. Run `latex` on `physconst.ins` to create the `.sty` file. e.g. `latex physconst.ins`. +1. Run `latex` on `physconst.ins` to create the `.sty` file. e.g. +`latex physconst.ins`. 1. The following steps apply only if you want the documentation (recommended). - 1. Run `latex` on `physconst.dtx` to create the `.pdf` file. e.g. `xelatex physconst.pdf`. - 1. Run `makeindex` to create the index, e.g. `makeindex -s gind.ist -o physconst.ind physconst.idx`. - 1. Run `makeindex` to create the change log, e.g. `makeindex -s gglo.ist -o physconst.gls physconst.glo`. - 1. Run `latex` on `physconst.dtx` to create the `.pdf` file with index and change log. e.g. `xelatex physconst.pdf`. - 1. Run `latex` on `physconst.dtx` to get the labels sorted out. e.g. `xelatex physconst.pdf`. - -Instructions that might help can be for windows can be found at [this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files). + 1. Run `latex` on `physconst.dtx` to create the `.pdf` file. e.g. +`xelatex physconst.pdf`. + 1. Run `makeindex` to create the index, e.g. +`makeindex -s gind.ist -o physconst.ind physconst.idx`. + 1. Run `makeindex` to create the change log, e.g. +`makeindex -s gglo.ist -o physconst.gls physconst.glo`. + 1. Run `latex` on `physconst.dtx` to create the `.pdf` file with index and +change log. e.g. `xelatex physconst.pdf`. + 1. Run `latex` on `physconst.dtx` to get the labels sorted out. e.g. +`xelatex physconst.pdf`. + +Instructions that might help can be for windows can be found at +[this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files). # Installation First build the project as described above. ## For a single project -1. Copy the `physconst.sty` into your project where your `.tex` files are located. +1. Copy the `physconst.sty` into your project where your `.tex` files are +located. ## for all users and projects ### Linux / Mac using make and xelatex 1. `make localinstall` ### Otherwise -Instructions that might help can be for windows can be found at [this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files). +Instructions that might help can be for windows can be found at +[this post on StackExchange](https://tex.stackexchange.com/questions/369921/loading-packages-with-ins-and-dtx-files). 1. Figure out where your LaTeX local packages are installed. 1. Create a directory named `physconst` in that location. 1. Copy the `.sty` file into the directory you just created. diff --git a/macros/latex/contrib/physconst/physconst.dtx b/macros/latex/contrib/physconst/physconst.dtx index 691a5fd901..7ade189381 100644 --- a/macros/latex/contrib/physconst/physconst.dtx +++ b/macros/latex/contrib/physconst/physconst.dtx @@ -133,7 +133,7 @@ % The normal macros are the ones that you will typically use, whose values are % determined by the choice of options when the package is invoked. % -% \subsection{Naming Convention} +% \subsubsection{Naming Convention} % % Each macro starts with a lower case `k' to indicate that it is a constant. % If the macro is of special units, e.g. eV, those units will be specified next. @@ -147,41 +147,136 @@ %\index{Mass|usage} % % \DescribeMacro{\kMassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>Electron|usage} % |\kMassElectron| is the mass of an electron. % % \DescribeMacro{\keVMassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>Electron>in eV|usage} % |\keVMassElectron| is the mass of an electron. % +% \DescribeMacro{\kMassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>Electron|usage} +% |\kMassElectronNumeric| is the numeric value of +% the mass of an electron. +% +% \DescribeMacro{\keVMassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>Electron>in eV|usage} +% |\keVMassElectronNumeric| is the numeric value of +% the mass of an electron. +% % \DescribeMacro{\kMassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>Proton|usage} % |\kMassProton| is the mass of a proton. % % \DescribeMacro{\keVMassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>Proton>in eV|usage} % |\keVMassProton| is the mass of a proton. % +% \DescribeMacro{\kMassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>Proton|usage} +% |\kMassProtonNumeric| is the numeric value of +% the mass of a proton. +% +% \DescribeMacro{\keVMassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>Proton>in eV|usage} +% |\keVMassProtonNumeric| is the numeric value of +% the mass of a proton. +% % \DescribeMacro{\kMassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>Hydrogen atom|usage} % |\kMassHydrogen| is the mass of a neutral hydrogen atom. % % \DescribeMacro{\keVMassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>Hydrogen atom>in eV|usage} % |\keVMassHydrogen| is the mass of a neutral hydrogen atom. % +% \DescribeMacro{\kMassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>Hydrogen atom|usage} +% |\kMassHydrogenNumeric| is the numeric value of +% the mass of a neutral hydrogen atom. +% +% \DescribeMacro{\keVMassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>Hydrogen atom>in eV|usage} +% |\keVMassHydrogenNumeric| is the numeric value of +% the mass of a neutral hydrogen atom. +% % \DescribeMacro{\kMassSun} % \index{Mass>Sun|usage} % |\kMassSun| is the mass of the Sun. % +% \DescribeMacro{\kMassSunNumeric} +% \index{Mass>Sun|usage} +% |\kMassSunNumeric| is the numeric value of +% the mass of the Sun. +% +% \DescribeMacro{\kMassEarth} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\kMassEarth| is the mass of the Earth. +% +% \DescribeMacro{\kMassEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\kMassEarthNumeric| is the numeric value of +% the mass of the Earth. +% +% \DescribeMacro{\kMassJupiter} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\kMassJupiter| is the mass of Jupiter. +% +% \DescribeMacro{\kMassJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\kMassJupiterNumeric| is the numeric value of +% the mass of Jupiter. +% % \DescribeMacro{\kMassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>amu|usage} % |\kMassAMU| is the mass of an atomic mass unit. % % \DescribeMacro{\keVMassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % \index{Mass>amu>in eV|usage} % |\keVMassAMU| is the mass of an atomic mass unit. % +% \DescribeMacro{\kMassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>amu|usage} +% |\kMassAMUNumeric| is the numeric value of +% the mass of an atomic mass unit. +% +% \DescribeMacro{\keVMassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% \index{Mass>amu>in eV|usage} +% |\keVMassAMUNumeric| is the numeric value of +% the mass of an atomic mass unit. +% % %\subsubsection{Charge} % @@ -192,14 +287,29 @@ % \index{Charge>Elementary|usage} % |\kChargeFundamental| is the fundamental charge. % +% \DescribeMacro{\kChargeFundamentalNumeric} +% \index{Charge>Elementary|usage} +% |\kChargeFundamentalNumeric| is the numeric value of +% the fundamental charge. +% % \DescribeMacro{\kChargeElectron} % \index{Charge>Electron|usage} % |\kChargeElectron| is the charge of an electron. % +% \DescribeMacro{\kChargeElectronNumeric} +% \index{Charge>Electron|usage} +% |\kChargeElectronNumeric| is the numeric value of +% the charge of an electron. +% % \DescribeMacro{\kChargeProton} % \index{Charge>Proton|usage} % |\kChargeProton| is the charge of a proton. % +% \DescribeMacro{\kChargeProtonNumeric} +% \index{Charge>Proton|usage} +% |\kChargeProtonNumeric| is the numeric value of +% the charge of a proton. +% % %\subsubsection{Distances and Lengths} % @@ -210,19 +320,58 @@ % \index{Distances and Lengths>Bohr Radius|usage} % |\kRadiusBohr| is Bohr radius of an atom. % +% \DescribeMacro{\kRadiusBohrNumeric} +% \index{Distances and Lengths>Bohr Radius|usage} +% |\kRadiusBohrNumeric| is the numeric value of +% Bohr radius of an atom. +% % \DescribeMacro{\kAstronomicalUnit} % \index{Distances and Lengths>Astronomical Unit|usage} % |\kAstronomicalUnit| is the astronomical unit (the average distance between % the Earth and the Sun). % +% \DescribeMacro{\kAstronomicalUnitNumeric} +% \index{Distances and Lengths>Astronomical Unit|usage} +% |\kAstronomicalUnitNumeric| is the numeric value of +% the astronomical unit (the average distance between the +% Earth and the Sun). +% % \DescribeMacro{\kParsec} % \index{Distances and Lengths>Parsec|usage} % |\kParsec| is the length of a parsec ($\frac{648000\au}{\pi}$). % +% \DescribeMacro{\kParsecNumeric} +% \index{Distances and Lengths>Parsec|usage} +% |\kParsecNumeric| is the numeric value of +% the length of a parsec ($\frac{648000\au}{\pi}$). +% % \DescribeMacro{\kRadiusSun} % \index{Distances and Lengths>Solar Radius|usage} % |\kRadiusSun| is the mean radius of the Sun. % +% \DescribeMacro{\kRadiusSunNumeric} +% \index{Distances and Lengths>Solar Radius|usage} +% |\kRadiusSunNumeric| is the numeric value of +% the mean radius of the Sun. +% +% \DescribeMacro{\kRadiusEarth} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\kRadiusEarth| is the mean radius of the Earth. +% +% \DescribeMacro{\kRadiusEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\kRadiusEarthNumeric| is the numeric value of +% the mean radius of the Earth. +% +% \DescribeMacro{\kRadiusJupiter} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\kRadiusJupiter| is the mean radius of Jupiter. +% +% \DescribeMacro{\kRadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\kRadiusJupiterNumeric| is the numeric value of +% the mean radius of Jupiter. +% % %\subsubsection{Energy, Power, and Luminosity} % @@ -237,10 +386,25 @@ % \index{Energy, Power, and Luminosity>Rydberg>in eV|usage} % |\keVRydberg| is the Rydberg energy (the binding energy of Hydrogen). % +% \DescribeMacro{\kRydbergNumeric} +% \index{Energy, Power, and Luminosity>Rydberg|usage} +% |\kRydbergNumeric| is the numeric value of +% the Rydberg energy (the binding energy of Hydrogen). +% +% \DescribeMacro{\keVRydbergNumeric} +% \index{Energy, Power, and Luminosity>Rydberg>in eV|usage} +% |\keVRydbergNumeric| is the numeric value of +% the Rydberg energy (the binding energy of Hydrogen). +% % \DescribeMacro{\kLuminositySun} % \index{Energy, Power, and Luminosity>Solar Luminosity|usage} % |\kLuminositySun| is the luminosity of the Sun. % +% \DescribeMacro{\kLuminositySunNumeric} +% \index{Energy, Power, and Luminosity>Solar Luminosity|usage} +% |\kLuminositySunNumeric| is the numeric value of +% the luminosity of the Sun. +% % %\subsubsection{Pressure} % @@ -248,13 +412,27 @@ %\index{Pressure|usage} % % \DescribeMacro{\kPressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} % \index{Pressure>Standard Atmosphere|usage} % |\kPressureAtmosphere| is the standard atmospheric pressure. % +% \DescribeMacro{\kPressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% \index{Pressure>Standard Atmosphere|usage} +% |\kPressureAtmosphereNumeric| is the numeric value of +% the standard atmospheric pressure. +% % \DescribeMacro{\kPressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} % \index{Pressure>Standard Pressure|usage} % |\kPressureStandard| is the standard atmospheric pressure. % +% \DescribeMacro{\kPressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% \index{Pressure>Standard Pressure|usage} +% |\kPressureStandardNumeric| is the numeric value of +% the standard atmospheric pressure. +% % %\subsubsection{Velocity, Speed and Acceleration} % @@ -265,11 +443,25 @@ % \index{Velocity, Speed and Acceleration>Speed of Light|usage} % |\kSpeedLight| is the speed of light. % +% \DescribeMacro{\kSpeedLightNumeric} +% \index{Velocity, Speed and Acceleration>Speed of Light|usage} +% |\kSpeedLightNumeric| is the numeric value of +% the speed of light. +% % \DescribeMacro{\kAccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} % \index{Velocity, Speed and Acceleration>Acceleration due to Gravity|usage} % |\kAccelGravity| is the accelertion due to gravity at the surface of the % Earth. % +% \DescribeMacro{\kAccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% \index{Velocity, Speed and Acceleration>Acceleration due to Gravity|usage} +% |\kAccelGravityNumeric| is the numeric value of +% the accelertion due to gravity at the surface of the Earth. +% % %\subsubsection{Other Constants} % @@ -277,21 +469,45 @@ %\index{Other Constants|usage} % % \DescribeMacro{\kCoulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % \index{Other Constants>Coulomb Constant|usage} % |\kCoulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$). % +% \DescribeMacro{\kCoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \index{Other Constants>Coulomb Constant|usage} +% |\kCoulombNumeric| is the numeric value of +% the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$). +% % \DescribeMacro{\kVacuumPermittivity} % \index{Other Constants>Vacuum Permittivity|usage} % |\kVacuumPermittivity| is the electric permittivity of the vacuum. % +% \DescribeMacro{\kVacuumPermittivityNumeric} +% \index{Other Constants>Vacuum Permittivity|usage} +% |\kVacuumPermittivityNumeric| is the numeric value of +% the electric permittivity of the vacuum. +% % \DescribeMacro{\kVacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % \index{Other Constants>Vacuum Permeability|usage} % |\kVacuumPermeability| is the magnetic permeability of the vacuum. % +% \DescribeMacro{\kVacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% \index{Other Constants>Vacuum Permeability|usage} +% |\kVacuumPermeabilityNumeric| is the numeric value of +% the magnetic permeability of the vacuum. +% % \DescribeMacro{\kVacuumImpedance} % \index{Other Constants>Vacuum Impedance|usage} % |\kVacuumImpedance| is the characteristic impedance of the vacuum. % +% \DescribeMacro{\kVacuumImpedanceNumeric} +% \index{Other Constants>Vacuum Impedance|usage} +% |\kVacuumImpedanceNumeric| is the numeric value of +% the characteristic impedance of the vacuum. +% % \DescribeMacro{\kBoltzmann} % \index{Other Constants>Boltzmann|usage} % |\kBoltzmann| is the Boltzmann constant. @@ -300,50 +516,124 @@ % \index{Other Constants>Boltzmann>in eV|usage} % |\keVBoltzmann| is the Boltzmann constant. % +% \DescribeMacro{\kBoltzmannNumeric} +% \index{Other Constants>Boltzmann|usage} +% |\kBoltzmannNumeric| is the numeric value of +% the Boltzmann constant. +% +% \DescribeMacro{\keVBoltzmannNumeric} +% \index{Other Constants>Boltzmann>in eV|usage} +% |\keVBoltzmannNumeric| is the numeric value of +% the Boltzmann constant. +% % \DescribeMacro{\kPlanck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % \index{Other Constants>Planck|usage} % |\kPlanck| is the Planck constant. % % \DescribeMacro{\keVPlanck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % \index{Other Constants>Planck>in eV|usage} % |\keVPlanck| is the Planck constant. % +% \DescribeMacro{\kPlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \index{Other Constants>Planck|usage} +% |\kPlanckNumeric| is the numeric value of +% the Planck constant. +% +% \DescribeMacro{\keVPlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \index{Other Constants>Planck>in eV|usage} +% |\keVPlanckNumeric| is the numeric value of +% the Planck constant. +% % \DescribeMacro{\kPlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % \index{Other Constants>Reduced Planck|usage} % |\kPlanckReduced| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$. % % \DescribeMacro{\keVPlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % \index{Other Constants>Reduced Planck>in eV|usage} % |\keVPlanckReduced| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$. % +% \DescribeMacro{\kPlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \index{Other Constants>Reduced Planck|usage} +% |\kPlanckReducedNumeric| is the numeric value of +% the Reduced Planck constant $\left(\frac{h}{2\pi}\right)$. +% +% \DescribeMacro{\keVPlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \index{Other Constants>Reduced Planck>in eV|usage} +% |\keVPlanckReducedNumeric| is the numeric value of +% the Reduced Planck constant $\left(\frac{h}{2\pi}\right)$. +% % \DescribeMacro{\kGravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % \index{Other Constants>Newton's Gravitational Constant|usage} % |\kGravity| is Newton's gravitational constant. % +% \DescribeMacro{\kGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% \index{Other Constants>Newton's Gravitational Constant|usage} +% |\kGravityNumeric| is the numeric value of +% Newton's gravitational constant. +% % \DescribeMacro{\kStefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % \index{Other Constants>Stefan-Boltzmann|usage} % |\kStefanBoltzmann| is the Stefan-Boltzmann blackbody constant % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$. % +% \DescribeMacro{\kStefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \index{Other Constants>Stefan-Boltzmann|usage} +% |\kStefanBoltzmannNumeric| is the numeric value of +% the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$. +% % \DescribeMacro{\kRadiation} % \index{Other Constants>Radiation|usage} % |\kRadiation| is the radiation constant, $a % \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$. % +% \DescribeMacro{\kRadiationNumeric} +% \index{Other Constants>Radiation|usage} +% |\kRadiationNumeric| is the numeric value of +% the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$. +% % \DescribeMacro{\kFineStructure} % \index{Other Constants>Fine Structure|usage} % |\kFineStructure| is the fine structure constant. % +% \DescribeMacro{\kFineStructureNumeric} +% \index{Other Constants>Fine Structure|usage} +% |\kFineStructureNumeric| is the numeric value of +% the fine structure constant. +% % \DescribeMacro{\kFineStructureReciprocal} % \index{Other Constants>Fine Structure>Reciprocal|usage} % |\kFineStructureReciprocal| is the reciprocal of the fine structure constant. % +% \DescribeMacro{\kFineStructureReciprocalNumeric} +% \index{Other Constants>Fine Structure>Reciprocal|usage} +% |\kFineStructureReciprocalNumeric| is the numeric value of +% the reciprocal of the fine structure constant. +% % \DescribeMacro{\kAvogadro} % \index{Other Constants>Avogadro's Number|usage} % |\kAvogadro| is Avogadro's Number (the number of particles in a mole). % +% \DescribeMacro{\kAvogadroNumeric} +% \index{Other Constants>Avogadro's Number|usage} +% |\kAvogadroNumeric| is the numeric value of +% Avogadro's Number (the number of particles in a mole). +% % %\subsection{Detailed Macros} % @@ -353,7 +643,7 @@ % by physconst to define the macros that are normally used (those described % above. % -% \subsection{NamingConvention} +% \subsubsection{NamingConvention} % The detailed macros are named like \k@units@precision@name. The units % specify which units the constant is in (SI, cgs, or eV). For constants that % are independent of the unit system (e.g. Avogadro's number and the fine @@ -366,6 +656,8 @@ %\subsubsection{Mass} % % \DescribeMacro{\k@SI@short@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % |\k@SI@short@MassElectron| is the mass of an electron in SI units with % reduced precision. % (CODATA~2018) @@ -382,6 +674,8 @@ % \makeatother % % \DescribeMacro{\k@SI@full@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % |\k@SI@full@MassElectron| is the mass of an electron in SI units with full % precision. % (CODATA~2018) @@ -398,6 +692,8 @@ % \makeatother % % \DescribeMacro{\k@cgs@short@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % |\k@cgs@short@MassElectron| is the mass of an electron in cgs units with % reduced precision. % (CODATA~2018) @@ -414,6 +710,8 @@ % \makeatother % % \DescribeMacro{\k@cgs@full@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % |\k@cgs@full@MassElectron| is the mass of an electron in cgs units with full % precision. % (CODATA~2018) @@ -430,6 +728,8 @@ % \makeatother % % \DescribeMacro{\k@eV@short@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % |\k@eV@short@MassElectron| is the mass of an electron in eV with reduced % precision. % (CODATA~2018) @@ -446,6 +746,8 @@ % \makeatother % % \DescribeMacro{\k@eV@full@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} % |\k@eV@full@MassElectron| is the mass of an electron in eV with full % precision. % (CODATA~2018) @@ -461,2081 +763,8315 @@ % {The value is \k@eV@full@MassElectron}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@MassProton} -% |\k@SI@short@MassProton| is the mass of a proton in SI units with reduced +% \DescribeMacro{\k@SI@short@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassElectronNumeric| is a mathematical value of +% the mass of an electron in SI units with reduced % precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@MassProton\\ +% \textbackslash k@SI@short@MassElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@MassProton}\end{mdframed} +% {The value is \k@SI@short@MassElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@MassProton} -% |\k@SI@full@MassProton| is the mass of a proton in SI units with full +% \DescribeMacro{\k@SI@full@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassElectronNumeric| is a mathematical value of +% the mass of an electron in SI units with full % precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@MassProton\\ +% \textbackslash k@SI@full@MassElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@MassProton}\end{mdframed} +% {The value is \k@SI@full@MassElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@MassProton} -% |\k@cgs@short@MassProton| is the mass of a proton in cgs units with reduced +% \DescribeMacro{\k@cgs@short@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassElectronNumeric| is a mathematical value of +% the mass of an electron in cgs units with reduced % precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@MassProton\\ +% \textbackslash k@cgs@short@MassElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@MassProton}\end{mdframed} +% {The value is \k@cgs@short@MassElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@MassProton} -% |\k@cgs@full@MassProton| is the mass of a proton in cgs units with full +% \DescribeMacro{\k@cgs@full@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassElectronNumeric| is a mathematical value of +% the mass of an electron in cgs units with full % precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@MassProton\\ +% \textbackslash k@cgs@full@MassElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@MassProton}\end{mdframed} +% {The value is \k@cgs@full@MassElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@MassProton} -% |\k@eV@short@MassProton| is the mass of a proton in eV with reduced precision. +% \DescribeMacro{\k@eV@short@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassElectronNumeric| is a mathematical value of +% the mass of an electron in eV with reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@MassProton\\ +% \textbackslash k@eV@short@MassElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@MassProton}\end{mdframed} +% {The value is \k@eV@short@MassElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@MassProton} -% |\k@eV@full@MassProton| is the mass of a proton in eV with full precision. +% \DescribeMacro{\k@eV@full@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassElectronNumeric| is a mathematical value of +% the mass of an electron in eV with full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@MassProton\\ +% \textbackslash k@eV@full@MassElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@MassProton}\end{mdframed} +% {The value is \k@eV@full@MassElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@MassHydrogen} -% |\k@SI@short@MassHydrogen| is the mass of a neutral hydrogen atom in SI units -% with reduced precision. +% \DescribeMacro{\k@SI@short@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassProton| is the mass of a proton in SI units with reduced +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@MassHydrogen\\ +% \textbackslash k@SI@short@MassProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@MassHydrogen}\end{mdframed} +% {The value is \k@SI@short@MassProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@MassHydrogen} -% |\k@SI@full@MassHydrogen| is the mass of a neutral hydrogen atom in SI units -% with full precision. +% \DescribeMacro{\k@SI@full@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassProton| is the mass of a proton in SI units with full +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@MassHydrogen\\ +% \textbackslash k@SI@full@MassProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@MassHydrogen}\end{mdframed} +% {The value is \k@SI@full@MassProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@MassHydrogen} -% |\k@cgs@short@MassHydrogen| is the mass of a neutral hydrogen atom in cgs -% units with reduced precision. +% \DescribeMacro{\k@cgs@short@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassProton| is the mass of a proton in cgs units with reduced +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@MassHydrogen\\ +% \textbackslash k@cgs@short@MassProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@MassHydrogen}\end{mdframed} +% {The value is \k@cgs@short@MassProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@MassHydrogen} -% |\k@cgs@full@MassHydrogen| is the mass of a neutral hydrogen atom in cgs -% units with full precision. +% \DescribeMacro{\k@cgs@full@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassProton| is the mass of a proton in cgs units with full +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@MassHydrogen\\ +% \textbackslash k@cgs@full@MassProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@MassHydrogen}\end{mdframed} +% {The value is \k@cgs@full@MassProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@MassHydrogen} -% |\k@eV@short@MassHydrogen| is the mass of a neutral hydrogen atom in eV with -% reduced precision. +% \DescribeMacro{\k@eV@short@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassProton| is the mass of a proton in eV with reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@MassHydrogen\\ +% \textbackslash k@eV@short@MassProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@MassHydrogen}\end{mdframed} +% {The value is \k@eV@short@MassProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@MassHydrogen} -% |\k@eV@full@MassHydrogen| is the mass of a neutral hydrogen atom in eV with -% full precision. +% \DescribeMacro{\k@eV@full@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassProton| is the mass of a proton in eV with full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@MassHydrogen\\ +% \textbackslash k@eV@full@MassProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@MassHydrogen}\end{mdframed} +% {The value is \k@eV@full@MassProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@MassSun} -% |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced +% \DescribeMacro{\k@SI@short@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassProtonNumeric| is a mathematical value of +% the mass of a proton in SI units with reduced % precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@MassSun\\ +% \textbackslash k@SI@short@MassProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@MassSun}\end{mdframed} +% {The value is \k@SI@short@MassProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@MassSun} -% |\k@SI@full@MassSun| is the mass of the Sun in SI units with full precision. -% (IAU~Resolution~B3~2015) +% \DescribeMacro{\k@SI@full@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassProtonNumeric| is a mathematical value of +% the mass of a proton in SI units with full precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@MassSun\\ +% \textbackslash k@SI@full@MassProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@MassSun}\end{mdframed} +% {The value is \k@SI@full@MassProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@MassSun} -% |\k@cgs@short@MassSun| is the mass of the Sun in cgs units with reduced +% \DescribeMacro{\k@cgs@short@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassProtonNumeric| is a mathematical value of +% the mass of a proton in cgs units with reduced % precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@MassSun\\ +% \textbackslash k@cgs@short@MassProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@MassSun}\end{mdframed} +% {The value is \k@cgs@short@MassProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@MassSun} -% |\k@cgs@full@MassSun| is the mass of the Sun in cgs units with full precision. -% (IAU~Resolution~B3~2015) +% \DescribeMacro{\k@cgs@full@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassProtonNumeric| is a mathematical value of +% the mass of a proton in cgs units with full precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@MassSun\\ +% \textbackslash k@cgs@full@MassProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@MassSun}\end{mdframed} +% {The value is \k@cgs@full@MassProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@MassAMU} -% |\k@SI@short@MassAMU| is the mass of an atomic mass unit in SI units with -% reduced precision. +% \DescribeMacro{\k@eV@short@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassProtonNumeric| is a mathematical value of +% the mass of a proton in eV with reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@MassAMU\\ +% \textbackslash k@eV@short@MassProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@MassAMU}\end{mdframed} +% {The value is \k@eV@short@MassProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@MassAMU} -% |\k@SI@full@MassAMU| is the mass of an atomic mass unit in SI units with full -% precision. +% \DescribeMacro{\k@eV@full@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassProtonNumeric| is a mathematical value of +% the mass of a proton in eV with full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@MassAMU\\ +% \textbackslash k@eV@full@MassProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@MassAMU}\end{mdframed} +% {The value is \k@eV@full@MassProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@MassAMU} -% |\k@cgs@short@MassAMU| is the mass of an atomic mass unit in cgs units with -% reduced precision. +% \DescribeMacro{\k@SI@short@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassHydrogen| is the mass of a neutral hydrogen atom in SI units +% with reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@MassAMU\\ +% \textbackslash k@SI@short@MassHydrogen\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@MassAMU}\end{mdframed} +% {The value is \k@SI@short@MassHydrogen}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@MassAMU} -% |\k@cgs@full@MassAMU| is the mass of an atomic mass unit in cgs units with -% full precision. +% \DescribeMacro{\k@SI@full@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassHydrogen| is the mass of a neutral hydrogen atom in SI units +% with full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@MassAMU\\ +% \textbackslash k@SI@full@MassHydrogen\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@MassAMU}\end{mdframed} +% {The value is \k@SI@full@MassHydrogen}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@MassAMU} -% |\k@eV@short@MassAMU| is the mass of an atomic mass unit in eV with reduced -% precision. +% \DescribeMacro{\k@cgs@short@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassHydrogen| is the mass of a neutral hydrogen atom in cgs +% units with reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@MassAMU\\ +% \textbackslash k@cgs@short@MassHydrogen\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@MassAMU}\end{mdframed} +% {The value is \k@cgs@short@MassHydrogen}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@MassAMU} -% |\k@eV@full@MassAMU| is the mass of an atomic mass unit in eV with full -% precision. +% \DescribeMacro{\k@cgs@full@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassHydrogen| is the mass of a neutral hydrogen atom in cgs +% units with full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@MassAMU\\ +% \textbackslash k@cgs@full@MassHydrogen\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@MassAMU}\end{mdframed} +% {The value is \k@cgs@full@MassHydrogen}\end{mdframed} % \makeatother % -% -%\subsubsection{Charge} -% -% \DescribeMacro{\k@SI@short@ChargeFundamental} -% |\k@SI@short@ChargeFundamental| is the fundamental charge in SI units with +% \DescribeMacro{\k@eV@short@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassHydrogen| is the mass of a neutral hydrogen atom in eV with % reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@ChargeFundamental\\ +% \textbackslash k@eV@short@MassHydrogen\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@ChargeFundamental}\end{mdframed} +% {The value is \k@eV@short@MassHydrogen}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@ChargeFundamental} -% |\k@SI@full@ChargeFundamental| is the fundamental charge in SI units with +% \DescribeMacro{\k@eV@full@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassHydrogen| is the mass of a neutral hydrogen atom in eV with % full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@ChargeFundamental\\ +% \textbackslash k@eV@full@MassHydrogen\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@ChargeFundamental}\end{mdframed} +% {The value is \k@eV@full@MassHydrogen}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@ChargeFundamental} -% |\k@cgs@short@ChargeFundamental| is the fundamental charge in cgs units with +% \DescribeMacro{\k@SI@short@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassHydrogenNumeric| is a mathematical value of +% the mass of a neutral hydrogen atom in SI units with % reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@ChargeFundamental\\ +% \textbackslash k@SI@short@MassHydrogenNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@ChargeFundamental}\end{mdframed} +% {The value is \k@SI@short@MassHydrogenNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@ChargeFundamental} -% |\k@cgs@full@ChargeFundamental| is the fundamental charge in cgs units with +% \DescribeMacro{\k@SI@full@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassHydrogenNumeric| is a mathematical value of +% the mass of a neutral hydrogen atom in SI units with % full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@ChargeFundamental\\ +% \textbackslash k@SI@full@MassHydrogenNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@ChargeFundamental}\end{mdframed} +% {The value is \k@SI@full@MassHydrogenNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@ChargeElectron} -% |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with -% reduced precision. +% \DescribeMacro{\k@cgs@short@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassHydrogenNumeric| is a mathematical value of +% the mass of a neutral hydrogen atom in cgs units +% with reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@ChargeElectron\\ +% \textbackslash k@cgs@short@MassHydrogenNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@ChargeElectron}\end{mdframed} +% {The value is \k@cgs@short@MassHydrogenNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@ChargeElectron} -% |\k@SI@full@ChargeElectron| is the charge of an electron in SI units with -% full precision. +% \DescribeMacro{\k@cgs@full@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassHydrogenNumeric| is a mathematical value of +% the mass of a neutral hydrogen atom in cgs units +% with full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@ChargeElectron\\ +% \textbackslash k@cgs@full@MassHydrogenNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@ChargeElectron}\end{mdframed} +% {The value is \k@cgs@full@MassHydrogenNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@ChargeElectron} -% |\k@cgs@short@ChargeElectron| is the charge of an electron in cgs units with +% \DescribeMacro{\k@eV@short@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassHydrogenNumeric| is a mathematical value of +% the mass of a neutral hydrogen atom in eV with % reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@ChargeElectron\\ +% \textbackslash k@eV@short@MassHydrogenNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@ChargeElectron}\end{mdframed} +% {The value is \k@eV@short@MassHydrogenNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@ChargeElectron} -% |\k@cgs@full@ChargeElectron| is the charge of an electron in cgs units with -% full precision. +% \DescribeMacro{\k@eV@full@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassHydrogenNumeric| is a mathematical value of +% the mass of a neutral hydrogen atom in eV with full +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@ChargeElectron\\ +% \textbackslash k@eV@full@MassHydrogenNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@ChargeElectron}\end{mdframed} +% {The value is \k@eV@full@MassHydrogenNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@ChargeProton} -% |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced +% \DescribeMacro{\k@SI@short@MassSun} +% |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced % precision. -% (CODATA~2018) +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@ChargeProton\\ +% \textbackslash k@SI@short@MassSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@ChargeProton}\end{mdframed} +% {The value is \k@SI@short@MassSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@ChargeProton} -% |\k@SI@full@ChargeProton| is the charge of a proton in SI units with full -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@MassSun} +% |\k@SI@full@MassSun| is the mass of the Sun in SI units with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@ChargeProton\\ +% \textbackslash k@SI@full@MassSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@ChargeProton}\end{mdframed} +% {The value is \k@SI@full@MassSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@ChargeProton} -% |\k@cgs@short@ChargeProton| is the charge of a proton in cgs units with -% reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@MassSun} +% |\k@cgs@short@MassSun| is the mass of the Sun in cgs units with reduced +% precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@ChargeProton\\ +% \textbackslash k@cgs@short@MassSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@ChargeProton}\end{mdframed} +% {The value is \k@cgs@short@MassSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@ChargeProton} -% |\k@cgs@full@ChargeProton| is the charge of a proton in cgs units with full -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@full@MassSun} +% |\k@cgs@full@MassSun| is the mass of the Sun in cgs units with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@ChargeProton\\ +% \textbackslash k@cgs@full@MassSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@ChargeProton}\end{mdframed} +% {The value is \k@cgs@full@MassSun}\end{mdframed} % \makeatother % -% -%\subsubsection{Distances and Lengths} -% -% \DescribeMacro{\k@SI@short@RadiusBohr} -% |\k@SI@short@RadiusBohr| is Bohr radius of an atom in SI units with reduced -% precision. -% (Calculated) +% \DescribeMacro{\k@SI@short@MassSunNumeric} +% |\k@SI@short@MassSunNumeric| is a mathematical value of +% the mass of the Sun in SI units with reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@RadiusBohr\\ +% \textbackslash k@SI@short@MassSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@RadiusBohr}\end{mdframed} +% {The value is \k@SI@short@MassSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@RadiusBohr} -% |\k@SI@full@RadiusBohr| is Bohr radius of an atom in SI units with full -% precision. -% (Calculated) +% \DescribeMacro{\k@SI@full@MassSunNumeric} +% |\k@SI@full@MassSunNumeric| is a mathematical value of +% the mass of the Sun in SI units with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@RadiusBohr\\ +% \textbackslash k@SI@full@MassSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@RadiusBohr}\end{mdframed} +% {The value is \k@SI@full@MassSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@RadiusBohr} -% |\k@cgs@short@RadiusBohr| is Bohr radius of an atom in cgs units with reduced -% precision. -% (Calculated) +% \DescribeMacro{\k@cgs@short@MassSunNumeric} +% |\k@cgs@short@MassSunNumeric| is a mathematical value of +% the mass of the Sun in cgs units with reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@RadiusBohr\\ +% \textbackslash k@cgs@short@MassSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@RadiusBohr}\end{mdframed} +% {The value is \k@cgs@short@MassSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@RadiusBohr} -% |\k@cgs@full@RadiusBohr| is Bohr radius of an atom in cgs units with full -% precision. -% (Calculated) +% \DescribeMacro{\k@cgs@full@MassSunNumeric} +% |\k@cgs@full@MassSunNumeric| is a mathematical value of +% the mass of the Sun in cgs units with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@RadiusBohr\\ +% \textbackslash k@cgs@full@MassSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@RadiusBohr}\end{mdframed} +% {The value is \k@cgs@full@MassSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@AstronomicalUnit} -% |\k@SI@short@AstronomicalUnit| is the astronomical unit (the average distance -% between the Earth and the Sun) in SI units with reduced precision. -% (IAU~Resolution~B2~2012) +% \DescribeMacro{\k@short@MassEarth} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@short@MassEarth| is the mass of the Earth with reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@AstronomicalUnit\\ +% \textbackslash k@short@MassEarth\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@AstronomicalUnit}\end{mdframed} +% {The value is \k@short@MassEarth}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@AstronomicalUnit} -% |\k@SI@full@AstronomicalUnit| is the astronomical unit (the average distance -% between the Earth and the Sun) in SI units with full precision. -% (IAU~Resolution~B2~2012) +% \DescribeMacro{\k@full@MassEarth} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@full@MassEarth| is the mass of the Earth with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@AstronomicalUnit\\ +% \textbackslash k@full@MassEarth\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@AstronomicalUnit}\end{mdframed} +% {The value is \k@full@MassEarth}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@AstronomicalUnit} -% |\k@cgs@short@AstronomicalUnit| is the astronomical unit (the average -% distance between the Earth and the Sun) in cgs units with reduced precision. -% (IAU~Resolution~B2~2012) +% \DescribeMacro{\k@short@MassEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@short@MassEarthNumeric| is a mathematical value of +% the mass of the Earth with reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@AstronomicalUnit\\ +% \textbackslash k@short@MassEarthNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@AstronomicalUnit}\end{mdframed} +% {The value is \k@short@MassEarthNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@AstronomicalUnit} -% |\k@cgs@full@AstronomicalUnit| is the astronomical unit (the average distance -% between the Earth and the Sun) in cgs units with full precision. -% (IAU~Resolution~B2~2012) +% \DescribeMacro{\k@full@MassEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@full@MassEarthNumeric| is a mathematical value of +% the mass of the Earth with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@AstronomicalUnit\\ +% \textbackslash k@full@MassEarthNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@AstronomicalUnit}\end{mdframed} +% {The value is \k@full@MassEarthNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@Parsec} -% |\k@SI@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in -% SI units with reduced precision. -% (Calculated) +% \DescribeMacro{\k@short@MassJupiter} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@short@MassJupiter| is the mass of Jupiter with reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Parsec\\ +% \textbackslash k@short@MassJupiter\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Parsec}\end{mdframed} +% {The value is \k@short@MassJupiter}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Parsec} -% |\k@SI@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in SI -% units with full precision. -% (Calculated) +% \DescribeMacro{\k@full@MassJupiter} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@full@MassJupiter| is the mass of Jupiter with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Parsec\\ +% \textbackslash k@full@MassJupiter\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Parsec}\end{mdframed} +% {The value is \k@full@MassJupiter}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Parsec} -% |\k@cgs@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in -% cgs units with reduced precision. -% (Calculated) +% \DescribeMacro{\k@short@MassJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@short@MassJupiterNumeric| is a mathematical value of +% the mass of Jupiter with reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Parsec\\ +% \textbackslash k@short@MassJupiterNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Parsec}\end{mdframed} +% {The value is \k@short@MassJupiterNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Parsec} -% |\k@cgs@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in -% cgs units with full precision. -% (Calculated) +% \DescribeMacro{\k@full@MassJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@full@MassJupiterNumeric| is a mathematical value of +% the mass of Jupiter with full precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Parsec\\ +% \textbackslash k@full@MassJupiterNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Parsec}\end{mdframed} +% {The value is \k@full@MassJupiterNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@RadiusSun} -% |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with +% \DescribeMacro{\k@SI@short@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassAMU| is the mass of an atomic mass unit in SI units with % reduced precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@RadiusSun\\ +% \textbackslash k@SI@short@MassAMU\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@RadiusSun}\end{mdframed} +% {The value is \k@SI@short@MassAMU}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@RadiusSun} -% |\k@SI@full@RadiusSun| is the mean radius of the Sun in SI units with full +% \DescribeMacro{\k@SI@full@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassAMU| is the mass of an atomic mass unit in SI units with full % precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@RadiusSun\\ +% \textbackslash k@SI@full@MassAMU\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@RadiusSun}\end{mdframed} +% {The value is \k@SI@full@MassAMU}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@RadiusSun} -% |\k@cgs@short@RadiusSun| is the mean radius of the Sun in cgs units with +% \DescribeMacro{\k@cgs@short@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassAMU| is the mass of an atomic mass unit in cgs units with % reduced precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@RadiusSun\\ +% \textbackslash k@cgs@short@MassAMU\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@RadiusSun}\end{mdframed} +% {The value is \k@cgs@short@MassAMU}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@RadiusSun} -% |\k@cgs@full@RadiusSun| is the mean radius of the Sun in cgs units with full -% precision. -% (IAU~Resolution~B3~2015) +% \DescribeMacro{\k@cgs@full@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassAMU| is the mass of an atomic mass unit in cgs units with +% full precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@RadiusSun\\ +% \textbackslash k@cgs@full@MassAMU\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@RadiusSun}\end{mdframed} +% {The value is \k@cgs@full@MassAMU}\end{mdframed} % \makeatother % -% -%\subsubsection{Energy, Power, and Luminosity} -% -% \DescribeMacro{\k@SI@short@Rydberg} -% |\k@SI@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in SI units with reduced precision. -% (Calculated) +% \DescribeMacro{\k@eV@short@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassAMU| is the mass of an atomic mass unit in eV with reduced +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Rydberg\\ +% \textbackslash k@eV@short@MassAMU\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Rydberg}\end{mdframed} +% {The value is \k@eV@short@MassAMU}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Rydberg} -% |\k@SI@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in SI units with full precision. -% (Calculated) +% \DescribeMacro{\k@eV@full@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassAMU| is the mass of an atomic mass unit in eV with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Rydberg\\ +% \textbackslash k@eV@full@MassAMU\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Rydberg}\end{mdframed} +% {The value is \k@eV@full@MassAMU}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Rydberg} -% |\k@cgs@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in cgs units with reduced precision. -% (Calculated) +% \DescribeMacro{\k@SI@short@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassAMUNumeric| is a mathematical value of +% the mass of an atomic mass unit in SI units with reduced +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Rydberg\\ +% \textbackslash k@SI@short@MassAMUNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Rydberg}\end{mdframed} +% {The value is \k@SI@short@MassAMUNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Rydberg} -% |\k@cgs@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in cgs units with full precision. -% (Calculated) +% \DescribeMacro{\k@SI@full@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassAMUNumeric| is a mathematical value of +% the mass of an atomic mass unit in SI units with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Rydberg\\ +% \textbackslash k@SI@full@MassAMUNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Rydberg}\end{mdframed} +% {The value is \k@SI@full@MassAMUNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@Rydberg} -% |\k@eV@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in eV with reduced precision. -% (Calculated) +% \DescribeMacro{\k@cgs@short@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassAMUNumeric| is a mathematical value of +% the mass of an atomic mass unit in cgs units with +% reduced precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@Rydberg\\ +% \textbackslash k@cgs@short@MassAMUNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@Rydberg}\end{mdframed} +% {The value is \k@cgs@short@MassAMUNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@Rydberg} -% |\k@eV@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in eV with full precision. -% (Calculated) +% \DescribeMacro{\k@cgs@full@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassAMUNumeric| is a mathematical value of +% the mass of an atomic mass unit in cgs units with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@Rydberg\\ +% \textbackslash k@cgs@full@MassAMUNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@Rydberg}\end{mdframed} +% {The value is \k@cgs@full@MassAMUNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@LuminositySun} -% |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with -% reduced precision. -% (IAU~Resolution~B3~2015) +% \DescribeMacro{\k@eV@short@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassAMUNumeric| is a mathematical value of +% the mass of an atomic mass unit in eV with reduced +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@LuminositySun\\ +% \textbackslash k@eV@short@MassAMUNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@LuminositySun}\end{mdframed} +% {The value is \k@eV@short@MassAMUNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@LuminositySun} -% |\k@SI@full@LuminositySun| is the luminosity of the Sun in SI units with full -% precision. -% (IAU~Resolution~B3~2015) +% \DescribeMacro{\k@eV@full@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassAMUNumeric| is a mathematical value of +% the mass of an atomic mass unit in eV with full precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@LuminositySun\\ +% \textbackslash k@eV@full@MassAMUNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@LuminositySun}\end{mdframed} +% {The value is \k@eV@full@MassAMUNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@LuminositySun} -% |\k@cgs@short@LuminositySun| is the luminosity of the Sun in cgs units with +% +%\subsubsection{Charge} +% +% \DescribeMacro{\k@SI@short@ChargeFundamental} +% |\k@SI@short@ChargeFundamental| is the fundamental charge in SI units with % reduced precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@LuminositySun\\ +% \textbackslash k@SI@short@ChargeFundamental\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@LuminositySun}\end{mdframed} +% {The value is \k@SI@short@ChargeFundamental}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@LuminositySun} -% |\k@cgs@full@LuminositySun| is the luminosity of the Sun in cgs units with +% \DescribeMacro{\k@SI@full@ChargeFundamental} +% |\k@SI@full@ChargeFundamental| is the fundamental charge in SI units with % full precision. -% (IAU~Resolution~B3~2015) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@LuminositySun\\ +% \textbackslash k@SI@full@ChargeFundamental\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@LuminositySun}\end{mdframed} +% {The value is \k@SI@full@ChargeFundamental}\end{mdframed} % \makeatother % -% -%\subsubsection{Pressure} -% -% \DescribeMacro{\k@SI@short@PressureAtmosphere} -% |\k@SI@short@PressureAtmosphere| is the standard atmospheric pressure in SI -% units with reduced precision. +% \DescribeMacro{\k@cgs@short@ChargeFundamental} +% |\k@cgs@short@ChargeFundamental| is the fundamental charge in cgs units with +% reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@PressureAtmosphere\\ +% \textbackslash k@cgs@short@ChargeFundamental\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@PressureAtmosphere}\end{mdframed} +% {The value is \k@cgs@short@ChargeFundamental}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@PressureAtmosphere} -% |\k@SI@full@PressureAtmosphere| is the standard atmospheric pressure in SI -% units with full precision. +% \DescribeMacro{\k@cgs@full@ChargeFundamental} +% |\k@cgs@full@ChargeFundamental| is the fundamental charge in cgs units with +% full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@PressureAtmosphere\\ +% \textbackslash k@cgs@full@ChargeFundamental\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@PressureAtmosphere}\end{mdframed} +% {The value is \k@cgs@full@ChargeFundamental}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@PressureAtmosphere} -% |\k@cgs@short@PressureAtmosphere| is the standard atmospheric pressure in cgs -% units with reduced precision. +% \DescribeMacro{\k@SI@short@ChargeFundamentalNumeric} +% |\k@SI@short@ChargeFundamentalNumeric| is a mathematical value of +% the fundamental charge in SI units with reduced +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@PressureAtmosphere\\ +% \textbackslash k@SI@short@ChargeFundamentalNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@PressureAtmosphere}\end{mdframed} +% {The value is \k@SI@short@ChargeFundamentalNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@PressureAtmosphere} -% |\k@cgs@full@PressureAtmosphere| is the standard atmospheric pressure in cgs -% units with full precision. +% \DescribeMacro{\k@SI@full@ChargeFundamentalNumeric} +% |\k@SI@full@ChargeFundamentalNumeric| is a mathematical value of +% the fundamental charge in SI units with full +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@PressureAtmosphere\\ +% \textbackslash k@SI@full@ChargeFundamentalNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@PressureAtmosphere}\end{mdframed} +% {The value is \k@SI@full@ChargeFundamentalNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@PressureStandard} -% |\k@SI@short@PressureStandard| is the standard atmospheric pressure in SI -% units with reduced precision. +% \DescribeMacro{\k@cgs@short@ChargeFundamentalNumeric} +% |\k@cgs@short@ChargeFundamentalNumeric| is a mathematical value of +% the fundamental charge in cgs units with +% reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@PressureStandard\\ +% \textbackslash k@cgs@short@ChargeFundamentalNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@PressureStandard}\end{mdframed} +% {The value is \k@cgs@short@ChargeFundamentalNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@PressureStandard} -% |\k@SI@full@PressureStandard| is the standard atmospheric pressure in SI -% units with full precision. +% \DescribeMacro{\k@cgs@full@ChargeFundamentalNumeric} +% |\k@cgs@full@ChargeFundamentalNumeric| is a mathematical value of +% the fundamental charge in cgs units with full +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@PressureStandard\\ +% \textbackslash k@cgs@full@ChargeFundamentalNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@PressureStandard}\end{mdframed} +% {The value is \k@cgs@full@ChargeFundamentalNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@PressureStandard} -% |\k@cgs@short@PressureStandard| is the standard atmospheric pressure in cgs -% units with reduced precision. +% \DescribeMacro{\k@SI@short@ChargeElectron} +% |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with +% reduced precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@PressureStandard\\ +% \textbackslash k@SI@short@ChargeElectron\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@PressureStandard}\end{mdframed} +% {The value is \k@SI@short@ChargeElectron}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@PressureStandard} -% |\k@cgs@full@PressureStandard| is the standard atmospheric pressure in cgs -% units with full precision. +% \DescribeMacro{\k@SI@full@ChargeElectron} +% |\k@SI@full@ChargeElectron| is the charge of an electron in SI units with +% full precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@PressureStandard\\ +% \textbackslash k@SI@full@ChargeElectron\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@PressureStandard}\end{mdframed} +% {The value is \k@SI@full@ChargeElectron}\end{mdframed} % \makeatother % -% -%\subsubsection{Velocity, Speed and Acceleration} -% -% \DescribeMacro{\k@SI@short@SpeedLight} -% |\k@SI@short@SpeedLight| is the speed of light in SI units with reduced -% precision. -% (CODATA 2018) +% \DescribeMacro{\k@cgs@short@ChargeElectron} +% |\k@cgs@short@ChargeElectron| is the charge of an electron in cgs units with +% reduced precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@SpeedLight\\ +% \textbackslash k@cgs@short@ChargeElectron\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@SpeedLight}\end{mdframed} +% {The value is \k@cgs@short@ChargeElectron}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@SpeedLight} -% |\k@SI@full@SpeedLight| is the speed of light in SI units with full precision. -% (CODATA 2018) +% \DescribeMacro{\k@cgs@full@ChargeElectron} +% |\k@cgs@full@ChargeElectron| is the charge of an electron in cgs units with +% full precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@SpeedLight\\ +% \textbackslash k@cgs@full@ChargeElectron\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@SpeedLight}\end{mdframed} +% {The value is \k@cgs@full@ChargeElectron}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@SpeedLight} -% |\k@cgs@short@SpeedLight| is the speed of light in cgs units with reduced +% \DescribeMacro{\k@SI@short@ChargeElectronNumeric} +% |\k@SI@short@ChargeElectronNumeric| is a mathematical value of +% the charge of an electron in SI units with reduced % precision. -% (CODATA 2018) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@SpeedLight\\ +% \textbackslash k@SI@short@ChargeElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@SpeedLight}\end{mdframed} +% {The value is \k@SI@short@ChargeElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@SpeedLight} -% |\k@cgs@full@SpeedLight| is the speed of light in cgs units with full +% \DescribeMacro{\k@SI@full@ChargeElectronNumeric} +% |\k@SI@full@ChargeElectronNumeric| is a mathematical value of +% the charge of an electron in SI units with full % precision. -% (CODATA 2018) +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@SpeedLight\\ +% \textbackslash k@SI@full@ChargeElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@SpeedLight}\end{mdframed} +% {The value is \k@SI@full@ChargeElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@AccelGravity} -% |\k@SI@short@AccelGravity| is the accelertion due to gravity at the surface -% of the Earth in SI units with reduced precision. -% (CODATA 2018) +% \DescribeMacro{\k@cgs@short@ChargeElectronNumeric} +% |\k@cgs@short@ChargeElectronNumeric| is a mathematical value of +% the charge of an electron in cgs units with +% reduced precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@AccelGravity\\ +% \textbackslash k@cgs@short@ChargeElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@AccelGravity}\end{mdframed} +% {The value is \k@cgs@short@ChargeElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@AccelGravity} -% |\k@SI@full@AccelGravity| is the accelertion due to gravity at the surface of -% the Earth in SI units with full precision. -% (CODATA 2018) +% \DescribeMacro{\k@cgs@full@ChargeElectronNumeric} +% |\k@cgs@full@ChargeElectronNumeric| is a mathematical value of +% the charge of an electron in cgs units with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@AccelGravity\\ +% \textbackslash k@cgs@full@ChargeElectronNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@AccelGravity}\end{mdframed} +% {The value is \k@cgs@full@ChargeElectronNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@AccelGravity} -% |\k@cgs@short@AccelGravity| is the accelertion due to gravity at the surface -% of the Earth in cgs units with reduced precision. -% (CODATA 2018) +% \DescribeMacro{\k@SI@short@ChargeProton} +% |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@AccelGravity\\ +% \textbackslash k@SI@short@ChargeProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@AccelGravity}\end{mdframed} +% {The value is \k@SI@short@ChargeProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@AccelGravity} -% |\k@cgs@full@AccelGravity| is the accelertion due to gravity at the surface -% of the Earth in cgs units with full precision. -% (CODATA 2018) +% \DescribeMacro{\k@SI@full@ChargeProton} +% |\k@SI@full@ChargeProton| is the charge of a proton in SI units with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@AccelGravity\\ +% \textbackslash k@SI@full@ChargeProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@AccelGravity}\end{mdframed} +% {The value is \k@SI@full@ChargeProton}\end{mdframed} % \makeatother % -% -%\subsubsection{Other Constants} -% -% \DescribeMacro{\k@SI@short@Coulomb} -% |\k@SI@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in -% SI units with reduced precision. -% (Calculated) +% \DescribeMacro{\k@cgs@short@ChargeProton} +% |\k@cgs@short@ChargeProton| is the charge of a proton in cgs units with +% reduced precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Coulomb\\ +% \textbackslash k@cgs@short@ChargeProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Coulomb}\end{mdframed} +% {The value is \k@cgs@short@ChargeProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Coulomb} -% |\k@SI@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in -% SI units with full precision. -% (Calculated) +% \DescribeMacro{\k@cgs@full@ChargeProton} +% |\k@cgs@full@ChargeProton| is the charge of a proton in cgs units with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Coulomb\\ +% \textbackslash k@cgs@full@ChargeProton\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Coulomb}\end{mdframed} +% {The value is \k@cgs@full@ChargeProton}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Coulomb} -% |\k@cgs@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) -% in cgs units with reduced precision. -% (Calculated) +% \DescribeMacro{\k@SI@short@ChargeProtonNumeric} +% |\k@SI@short@ChargeProtonNumeric| is a mathematical value of +% the charge of a proton in SI units with reduced +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Coulomb\\ +% \textbackslash k@SI@short@ChargeProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Coulomb}\end{mdframed} +% {The value is \k@SI@short@ChargeProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Coulomb} -% |\k@cgs@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in -% cgs units with full precision. -% (Calculated) +% \DescribeMacro{\k@SI@full@ChargeProtonNumeric} +% |\k@SI@full@ChargeProtonNumeric| is a mathematical value of +% the charge of a proton in SI units with full +% precision. +% (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Coulomb\\ +% \textbackslash k@SI@full@ChargeProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Coulomb}\end{mdframed} +% {The value is \k@SI@full@ChargeProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@VacuumPermittivity} -% |\k@SI@short@VacuumPermittivity| is the electric permittivity of the vacuum -% in SI units with reduced precision. +% \DescribeMacro{\k@cgs@short@ChargeProtonNumeric} +% |\k@cgs@short@ChargeProtonNumeric| is a mathematical value of +% the charge of a proton in cgs units with reduced +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@VacuumPermittivity\\ +% \textbackslash k@cgs@short@ChargeProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@VacuumPermittivity}\end{mdframed} +% {The value is \k@cgs@short@ChargeProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@VacuumPermittivity} -% |\k@SI@full@VacuumPermittivity| is the electric permittivity of the vacuum in -% SI units with full precision. +% \DescribeMacro{\k@cgs@full@ChargeProtonNumeric} +% |\k@cgs@full@ChargeProtonNumeric| is a mathematical value of +% the charge of a proton in cgs units with full +% precision. % (CODATA~2018) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@VacuumPermittivity\\ +% \textbackslash k@cgs@full@ChargeProtonNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@VacuumPermittivity}\end{mdframed} +% {The value is \k@cgs@full@ChargeProtonNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@VacuumPermittivity} -% |\k@cgs@short@VacuumPermittivity| is the electric permittivity of the vacuum -% in cgs units with reduced precision. -% (CODATA~2018) % -% The macro can be invoked by (e.g.) -% \begin{mdframed}[backgroundcolor=orange!25]% -% {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@VacuumPermittivity\\ -% \textbackslash makeatother}}\end{mdframed} -% \makeatletter -% Resulting in -% \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@VacuumPermittivity}\end{mdframed} -% \makeatother +%\subsubsection{Distances and Lengths} % -% \DescribeMacro{\k@cgs@full@VacuumPermittivity} -% |\k@cgs@full@VacuumPermittivity| is the electric permittivity of the vacuum -% in cgs units with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@short@RadiusBohr} +% |\k@SI@short@RadiusBohr| is Bohr radius of an atom in SI units with reduced +% precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@VacuumPermittivity\\ +% \textbackslash k@SI@short@RadiusBohr\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@VacuumPermittivity}\end{mdframed} +% {The value is \k@SI@short@RadiusBohr}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@VacuumPermeability} -% |\k@SI@short@VacuumPermeability| is the magnetic permeability of the vacuum -% in SI units with reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@RadiusBohr} +% |\k@SI@full@RadiusBohr| is Bohr radius of an atom in SI units with full +% precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@VacuumPermeability\\ +% \textbackslash k@SI@full@RadiusBohr\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@VacuumPermeability}\end{mdframed} +% {The value is \k@SI@full@RadiusBohr}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@VacuumPermeability} -% |\k@SI@full@VacuumPermeability| is the magnetic permeability of the vacuum in -% SI units with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@RadiusBohr} +% |\k@cgs@short@RadiusBohr| is Bohr radius of an atom in cgs units with reduced +% precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@VacuumPermeability\\ +% \textbackslash k@cgs@short@RadiusBohr\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@VacuumPermeability}\end{mdframed} +% {The value is \k@cgs@short@RadiusBohr}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@VacuumPermeability} -% |\k@cgs@short@VacuumPermeability| is the magnetic permeability of the vacuum -% in cgs units with reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@full@RadiusBohr} +% |\k@cgs@full@RadiusBohr| is Bohr radius of an atom in cgs units with full +% precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@VacuumPermeability\\ +% \textbackslash k@cgs@full@RadiusBohr\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@VacuumPermeability}\end{mdframed} +% {The value is \k@cgs@full@RadiusBohr}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@VacuumPermeability} -% |\k@cgs@full@VacuumPermeability| is the magnetic permeability of the vacuum -% in cgs units with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@short@RadiusBohrNumeric} +% |\k@SI@short@RadiusBohrNumeric| is a mathematical value of +% Bohr radius of an atom in SI units with reduced +% precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@VacuumPermeability\\ +% \textbackslash k@SI@short@RadiusBohrNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@VacuumPermeability}\end{mdframed} +% {The value is \k@SI@short@RadiusBohrNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@short@VacuumImpedance} -% |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with -% reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@RadiusBohrNumeric} +% |\k@SI@full@RadiusBohrNumeric| is a mathematical value of +% Bohr radius of an atom in SI units with full precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@short@VacuumImpedance\\ +% \textbackslash k@SI@full@RadiusBohrNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@short@VacuumImpedance}\end{mdframed} +% {The value is \k@SI@full@RadiusBohrNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@full@VacuumImpedance} -% |\k@full@VacuumImpedance| is the characteristic impedance of the vacuum with -% full precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@RadiusBohrNumeric} +% |\k@cgs@short@RadiusBohrNumeric| is a mathematical value of +% Bohr radius of an atom in cgs units with reduced +% precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@full@VacuumImpedance\\ +% \textbackslash k@cgs@short@RadiusBohrNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@full@VacuumImpedance}\end{mdframed} +% {The value is \k@cgs@short@RadiusBohrNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@Boltzmann} -% |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced +% \DescribeMacro{\k@cgs@full@RadiusBohrNumeric} +% |\k@cgs@full@RadiusBohrNumeric| is a mathematical value of +% Bohr radius of an atom in cgs units with full % precision. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Boltzmann\\ +% \textbackslash k@cgs@full@RadiusBohrNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Boltzmann}\end{mdframed} +% {The value is \k@cgs@full@RadiusBohrNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Boltzmann} -% |\k@SI@full@Boltzmann| is the Boltzmann constant in SI units with full -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@short@AstronomicalUnit} +% |\k@SI@short@AstronomicalUnit| is the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with reduced precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Boltzmann\\ +% \textbackslash k@SI@short@AstronomicalUnit\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Boltzmann}\end{mdframed} +% {The value is \k@SI@short@AstronomicalUnit}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Boltzmann} -% |\k@cgs@short@Boltzmann| is the Boltzmann constant in cgs units with reduced -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@AstronomicalUnit} +% |\k@SI@full@AstronomicalUnit| is the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with full precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Boltzmann\\ +% \textbackslash k@SI@full@AstronomicalUnit\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Boltzmann}\end{mdframed} +% {The value is \k@SI@full@AstronomicalUnit}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Boltzmann} -% |\k@cgs@full@Boltzmann| is the Boltzmann constant in cgs units with full -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@AstronomicalUnit} +% |\k@cgs@short@AstronomicalUnit| is the astronomical unit (the average +% distance between the Earth and the Sun) in cgs units with reduced precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Boltzmann\\ +% \textbackslash k@cgs@short@AstronomicalUnit\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Boltzmann}\end{mdframed} +% {The value is \k@cgs@short@AstronomicalUnit}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@Boltzmann} -% |\k@eV@short@Boltzmann| is the Boltzmann constant in eV with reduced -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@full@AstronomicalUnit} +% |\k@cgs@full@AstronomicalUnit| is the astronomical unit (the average distance +% between the Earth and the Sun) in cgs units with full precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@Boltzmann\\ +% \textbackslash k@cgs@full@AstronomicalUnit\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@Boltzmann}\end{mdframed} +% {The value is \k@cgs@full@AstronomicalUnit}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@Boltzmann} -% |\k@eV@full@Boltzmann| is the Boltzmann constant in eV with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@short@AstronomicalUnitNumeric} +% |\k@SI@short@AstronomicalUnitNumeric| is a mathematical value of +% the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with reduced precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@Boltzmann\\ +% \textbackslash k@SI@short@AstronomicalUnitNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@Boltzmann}\end{mdframed} +% {The value is \k@SI@short@AstronomicalUnitNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@Planck} -% |\k@SI@short@Planck| is the Planck constant in SI units with reduced -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@AstronomicalUnitNumeric} +% |\k@SI@full@AstronomicalUnitNumeric| is a mathematical value of +% the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with full precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Planck\\ +% \textbackslash k@SI@full@AstronomicalUnitNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Planck}\end{mdframed} +% {The value is \k@SI@full@AstronomicalUnitNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Planck} -% |\k@SI@full@Planck| is the Planck constant in SI units with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@AstronomicalUnitNumeric} +% |\k@cgs@short@AstronomicalUnitNumeric| is a mathematical value of +% the astronomical unit (the average distance +% between the Earth and the Sun) in cgs units with reduced precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Planck\\ +% \textbackslash k@cgs@short@AstronomicalUnitNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Planck}\end{mdframed} +% {The value is \k@cgs@short@AstronomicalUnitNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Planck} -% |\k@cgs@short@Planck| is the Planck constant in cgs units with reduced -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@full@AstronomicalUnitNumeric} +% |\k@cgs@full@AstronomicalUnitNumeric| is a mathematical value of +% the astronomical unit (the average distance +% between the Earth and the Sun) in cgs units with full precision. +% (IAU~Resolution~B2~2012) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Planck\\ +% \textbackslash k@cgs@full@AstronomicalUnitNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Planck}\end{mdframed} +% {The value is \k@cgs@full@AstronomicalUnitNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Planck} -% |\k@cgs@full@Planck| is the Planck constant in cgs units with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@short@Parsec} +% |\k@SI@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% SI units with reduced precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Planck\\ +% \textbackslash k@SI@short@Parsec\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Planck}\end{mdframed} +% {The value is \k@SI@short@Parsec}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@Planck} -% |\k@eV@short@Planck| is the Planck constant in eV with reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@Parsec} +% |\k@SI@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in SI +% units with full precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@Planck\\ +% \textbackslash k@SI@full@Parsec\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@Planck}\end{mdframed} +% {The value is \k@SI@full@Parsec}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@Planck} -% |\k@eV@full@Planck| is the Planck constant in eV with full precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@Parsec} +% |\k@cgs@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% cgs units with reduced precision. +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@Planck\\ +% \textbackslash k@cgs@short@Parsec\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@Planck}\end{mdframed} +% {The value is \k@cgs@short@Parsec}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@PlanckReduced} -% |\k@SI@short@PlanckReduced| is the Reduced Planck constant -% $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision. +% \DescribeMacro{\k@cgs@full@Parsec} +% |\k@cgs@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% cgs units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@PlanckReduced\\ +% \textbackslash k@cgs@full@Parsec\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@PlanckReduced}\end{mdframed} +% {The value is \k@cgs@full@Parsec}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@PlanckReduced} -% |\k@SI@full@PlanckReduced| is the Reduced Planck constant -% $\left(\frac{h}{2\pi}\right)$ in SI units with full precision. +% \DescribeMacro{\k@SI@short@ParsecNumeric} +% |\k@SI@short@ParsecNumeric| is a mathematical value of +% the length of a parsec ($\frac{648000\au}{\pi}$) in SI +% units with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@PlanckReduced\\ +% \textbackslash k@SI@short@ParsecNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@PlanckReduced}\end{mdframed} +% {The value is \k@SI@short@ParsecNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@PlanckReduced} -% |\k@cgs@short@PlanckReduced| is the Reduced Planck constant -% $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision. +% \DescribeMacro{\k@SI@full@ParsecNumeric} +% |\k@SI@full@ParsecNumeric| is a mathematical value of +% the length of a parsec ($\frac{648000\au}{\pi}$) in SI +% units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@PlanckReduced\\ +% \textbackslash k@SI@full@ParsecNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@PlanckReduced}\end{mdframed} +% {The value is \k@SI@full@ParsecNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@PlanckReduced} -% |\k@cgs@full@PlanckReduced| is the Reduced Planck constant -% $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision. +% \DescribeMacro{\k@cgs@short@ParsecNumeric} +% |\k@cgs@short@ParsecNumeric| is a mathematical value of +% the length of a parsec ($\frac{648000\au}{\pi}$) in cgs +% units with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@PlanckReduced\\ +% \textbackslash k@cgs@short@ParsecNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@PlanckReduced}\end{mdframed} +% {The value is \k@cgs@short@ParsecNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@short@PlanckReduced} -% |\k@eV@short@PlanckReduced| is the Reduced Planck constant -% $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision. +% \DescribeMacro{\k@cgs@full@ParsecNumeric} +% |\k@cgs@full@ParsecNumeric| is a mathematical value of +% the length of a parsec ($\frac{648000\au}{\pi}$) in cgs +% units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@short@PlanckReduced\\ +% \textbackslash k@cgs@full@ParsecNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@short@PlanckReduced}\end{mdframed} +% {The value is \k@cgs@full@ParsecNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@eV@full@PlanckReduced} -% |\k@eV@full@PlanckReduced| is the Reduced Planck constant -% $\left(\frac{h}{2\pi}\right)$ in eV with full precision. -% (Calculated) +% \DescribeMacro{\k@SI@short@RadiusSun} +% |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with +% reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@eV@full@PlanckReduced\\ +% \textbackslash k@SI@short@RadiusSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@eV@full@PlanckReduced}\end{mdframed} +% {The value is \k@SI@short@RadiusSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@Gravity} -% |\k@SI@short@Gravity| is Newton's gravitational constant in SI units with -% reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@full@RadiusSun} +% |\k@SI@full@RadiusSun| is the mean radius of the Sun in SI units with full +% precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Gravity\\ +% \textbackslash k@SI@full@RadiusSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Gravity}\end{mdframed} +% {The value is \k@SI@full@RadiusSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Gravity} -% |\k@SI@full@Gravity| is Newton's gravitational constant in SI units with full -% precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@short@RadiusSun} +% |\k@cgs@short@RadiusSun| is the mean radius of the Sun in cgs units with +% reduced precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Gravity\\ +% \textbackslash k@cgs@short@RadiusSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Gravity}\end{mdframed} +% {The value is \k@cgs@short@RadiusSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Gravity} -% |\k@cgs@short@Gravity| is Newton's gravitational constant in cgs units with -% reduced precision. -% (CODATA~2018) +% \DescribeMacro{\k@cgs@full@RadiusSun} +% |\k@cgs@full@RadiusSun| is the mean radius of the Sun in cgs units with full +% precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Gravity\\ +% \textbackslash k@cgs@full@RadiusSun\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Gravity}\end{mdframed} +% {The value is \k@cgs@full@RadiusSun}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Gravity} -% |\k@cgs@full@Gravity| is Newton's gravitational constant in cgs units with -% full precision. -% (CODATA~2018) +% \DescribeMacro{\k@SI@short@RadiusSunNumeric} +% |\k@SI@short@RadiusSunNumeric| is a mathematical value of +% the mean radius of the Sun in SI units with reduced +% precision. +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Gravity\\ +% \textbackslash k@SI@short@RadiusSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Gravity}\end{mdframed} +% {The value is \k@SI@short@RadiusSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@StefanBoltzmann} -% |\k@SI@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant -% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced +% \DescribeMacro{\k@SI@full@RadiusSunNumeric} +% |\k@SI@full@RadiusSunNumeric| is a mathematical value of +% the mean radius of the Sun in SI units with full % precision. -% (Calculated) +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@StefanBoltzmann\\ +% \textbackslash k@SI@full@RadiusSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@StefanBoltzmann}\end{mdframed} +% {The value is \k@SI@full@RadiusSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@StefanBoltzmann} -% |\k@SI@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant -% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full +% \DescribeMacro{\k@cgs@short@RadiusSunNumeric} +% |\k@cgs@short@RadiusSunNumeric| is a mathematical value of +% the mean radius of the Sun in cgs units with reduced % precision. -% (Calculated) +% (IAU~Resolution~B3~2015) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@StefanBoltzmann\\ +% \textbackslash k@cgs@short@RadiusSunNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@StefanBoltzmann}\end{mdframed} +% {The value is \k@cgs@short@RadiusSunNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@StefanBoltzmann} -% |\k@cgs@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant -% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced +% \DescribeMacro{\k@cgs@full@RadiusSunNumeric} +% |\k@cgs@full@RadiusSunNumeric| is a mathematical value of +% the mean radius of the Sun in cgs units with full % precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@RadiusSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@RadiusSunNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@RadiusEarth} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@short@RadiusEarth| is the mean radius of the Earth with reduced precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@RadiusEarth\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@RadiusEarth}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@RadiusEarth} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@full@RadiusEarth| is the mean radius of the Earth with full precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@RadiusEarth\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@RadiusEarth}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@RadiusEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@short@RadiusEarthNumeric| is a mathematical value of +% the mean radius of the Earth with reduced precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@RadiusEarthNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@RadiusEarthNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@RadiusEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@full@RadiusEarthNumeric| is a mathematical value of +% the mean radius of the Earth with full precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@RadiusEarthNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@RadiusEarthNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@RadiusJupiter} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@short@RadiusJupiter| is the mean radius of Jupiter with reduced precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@RadiusJupiter\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@RadiusJupiter}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@RadiusJupiter} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@full@RadiusJupiter| is the mean radius of Jupiter with full precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@RadiusJupiter\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@RadiusJupiter}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@RadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@short@RadiusJupiterNumeric| is a mathematical value of +% the mean radius of Jupiter with reduced precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@RadiusJupiterNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@RadiusJupiterNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@RadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@full@RadiusJupiterNumeric| is a mathematical value of +% the mean radius of Jupiter with full precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@RadiusJupiterNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@RadiusJupiterNumeric}\end{mdframed} +% \makeatother +% +% +%\subsubsection{Energy, Power, and Luminosity} +% +% \DescribeMacro{\k@SI@short@Rydberg} +% |\k@SI@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in SI units with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@StefanBoltzmann\\ +% \textbackslash k@SI@short@Rydberg\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@StefanBoltzmann}\end{mdframed} +% {The value is \k@SI@short@Rydberg}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@StefanBoltzmann} -% |\k@cgs@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant -% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full -% precision. +% \DescribeMacro{\k@SI@full@Rydberg} +% |\k@SI@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in SI units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@StefanBoltzmann\\ +% \textbackslash k@SI@full@Rydberg\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@StefanBoltzmann}\end{mdframed} +% {The value is \k@SI@full@Rydberg}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@short@Radiation} -% |\k@SI@short@Radiation| is the radiation constant, $a -% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced -% precision. +% \DescribeMacro{\k@cgs@short@Rydberg} +% |\k@cgs@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in cgs units with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@short@Radiation\\ +% \textbackslash k@cgs@short@Rydberg\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@short@Radiation}\end{mdframed} +% {The value is \k@cgs@short@Rydberg}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@SI@full@Radiation} -% |\k@SI@full@Radiation| is the radiation constant, $a -% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with full -% precision. +% \DescribeMacro{\k@cgs@full@Rydberg} +% |\k@cgs@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in cgs units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@SI@full@Radiation\\ +% \textbackslash k@cgs@full@Rydberg\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@SI@full@Radiation}\end{mdframed} +% {The value is \k@cgs@full@Rydberg}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@short@Radiation} -% |\k@cgs@short@Radiation| is the radiation constant, $a -% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with reduced -% precision. +% \DescribeMacro{\k@eV@short@Rydberg} +% |\k@eV@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in eV with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@short@Radiation\\ +% \textbackslash k@eV@short@Rydberg\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@short@Radiation}\end{mdframed} +% {The value is \k@eV@short@Rydberg}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@cgs@full@Radiation} -% |\k@cgs@full@Radiation| is the radiation constant, $a -% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with full -% precision. +% \DescribeMacro{\k@eV@full@Rydberg} +% |\k@eV@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in eV with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@cgs@full@Radiation\\ +% \textbackslash k@eV@full@Rydberg\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@cgs@full@Radiation}\end{mdframed} +% {The value is \k@eV@full@Rydberg}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@short@FineStructure} -% |\k@short@FineStructure| is the fine structure constant with reduced -% precision. +% \DescribeMacro{\k@SI@short@RydbergNumeric} +% |\k@SI@short@RydbergNumeric| is a mathematical value of +% the Rydberg energy (the binding energy of Hydrogen) in SI +% units with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@short@FineStructure\\ +% \textbackslash k@SI@short@RydbergNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@short@FineStructure}\end{mdframed} +% {The value is \k@SI@short@RydbergNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@full@FineStructure} -% |\k@full@FineStructure| is the fine structure constant with full precision. +% \DescribeMacro{\k@SI@full@RydbergNumeric} +% |\k@SI@full@RydbergNumeric| is a mathematical value of +% the Rydberg energy (the binding energy of Hydrogen) in SI +% units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@full@FineStructure\\ +% \textbackslash k@SI@full@RydbergNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@full@FineStructure}\end{mdframed} +% {The value is \k@SI@full@RydbergNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@short@FineStructureReciprocal} -% |\k@short@FineStructureReciprocal| is the reciprocal of the fine structure -% constant with reduced precision. +% \DescribeMacro{\k@cgs@short@RydbergNumeric} +% |\k@cgs@short@RydbergNumeric| is a mathematical value of +% the Rydberg energy (the binding energy of Hydrogen) in +% cgs units with reduced precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@short@FineStructureReciprocal\\ +% \textbackslash k@cgs@short@RydbergNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@short@FineStructureReciprocal}\end{mdframed} +% {The value is \k@cgs@short@RydbergNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@full@FineStructureReciprocal} -% |\k@full@FineStructureReciprocal| is the reciprocal of the fine structure -% constant with full precision. +% \DescribeMacro{\k@cgs@full@RydbergNumeric} +% |\k@cgs@full@RydbergNumeric| is a mathematical value of +% the Rydberg energy (the binding energy of Hydrogen) in +% cgs units with full precision. % (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@full@FineStructureReciprocal\\ +% \textbackslash k@cgs@full@RydbergNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@full@FineStructureReciprocal}\end{mdframed} +% {The value is \k@cgs@full@RydbergNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@short@Avogadro} -% |\k@short@Avogadro| is Avogadro's Number (the number of particles in a mole) +% \DescribeMacro{\k@eV@short@RydbergNumeric} +% |\k@eV@short@RydbergNumeric| is a mathematical value of +% the Rydberg energy (the binding energy of Hydrogen) in eV % with reduced precision. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@short@Avogadro\\ +% \textbackslash k@eV@short@RydbergNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@short@Avogadro}\end{mdframed} +% {The value is \k@eV@short@RydbergNumeric}\end{mdframed} % \makeatother % -% \DescribeMacro{\k@full@Avogadro} -% |\k@full@Avogadro| is Avogadro's Number (the number of particles in a mole) +% \DescribeMacro{\k@eV@full@RydbergNumeric} +% |\k@eV@full@RydbergNumeric| is a mathematical value of +% the Rydberg energy (the binding energy of Hydrogen) in eV % with full precision. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% % {\small\texttt{\textbackslash makeatletter\\ The value is -% \textbackslash k@full@Avogadro\\ +% \textbackslash k@eV@full@RydbergNumeric\\ % \textbackslash makeatother}}\end{mdframed} % \makeatletter % Resulting in % \begin{mdframed}[backgroundcolor=blue!25]% -% {The value is \k@full@Avogadro}\end{mdframed} +% {The value is \k@eV@full@RydbergNumeric}\end{mdframed} % \makeatother % -\makeatletter -% \StopEventually{} -% -% \section{Implementation} +% \DescribeMacro{\k@SI@short@LuminositySun} +% |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with +% reduced precision. +% (IAU~Resolution~B3~2015) % -% \subsection{Special} +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@LuminositySun\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@LuminositySun}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@LuminositySun} +% |\k@SI@full@LuminositySun| is the luminosity of the Sun in SI units with full +% precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@LuminositySun\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@LuminositySun}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@LuminositySun} +% |\k@cgs@short@LuminositySun| is the luminosity of the Sun in cgs units with +% reduced precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@LuminositySun\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@LuminositySun}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@LuminositySun} +% |\k@cgs@full@LuminositySun| is the luminosity of the Sun in cgs units with +% full precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@LuminositySun\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@LuminositySun}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@LuminositySunNumeric} +% |\k@SI@short@LuminositySunNumeric| is a mathematical value of +% the luminosity of the Sun in SI units with reduced +% precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@LuminositySunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@LuminositySunNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@LuminositySunNumeric} +% |\k@SI@full@LuminositySunNumeric| is a mathematical value of +% the luminosity of the Sun in SI units with full +% precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@LuminositySunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@LuminositySunNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@LuminositySunNumeric} +% |\k@cgs@short@LuminositySunNumeric| is a mathematical value of +% the luminosity of the Sun in cgs units with +% reduced precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@LuminositySunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@LuminositySunNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@LuminositySunNumeric} +% |\k@cgs@full@LuminositySunNumeric| is a mathematical value of +% the luminosity of the Sun in cgs units with full +% precision. +% (IAU~Resolution~B3~2015) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@LuminositySunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@LuminositySunNumeric}\end{mdframed} +% \makeatother +% +% +%\subsubsection{Pressure} +% +% \DescribeMacro{\k@SI@short@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureAtmosphere| is the standard atmospheric pressure in SI +% units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PressureAtmosphere\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PressureAtmosphere}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureAtmosphere| is the standard atmospheric pressure in SI +% units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PressureAtmosphere\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PressureAtmosphere}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureAtmosphere| is the standard atmospheric pressure in cgs +% units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PressureAtmosphere\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PressureAtmosphere}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureAtmosphere| is the standard atmospheric pressure in cgs +% units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PressureAtmosphere\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PressureAtmosphere}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureAtmosphereNumeric| is a mathematical value of +% the standard atmospheric pressure in SI units +% with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PressureAtmosphereNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PressureAtmosphereNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureAtmosphereNumeric| is a mathematical value of +% the standard atmospheric pressure in SI units +% with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PressureAtmosphereNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PressureAtmosphereNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureAtmosphereNumeric| is a mathematical value of +% the standard atmospheric pressure in cgs +% units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PressureAtmosphereNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PressureAtmosphereNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureAtmosphereNumeric| is a mathematical value of +% the standard atmospheric pressure in cgs units +% with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PressureAtmosphereNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PressureAtmosphereNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureStandard| is the standard atmospheric pressure in SI +% units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PressureStandard\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PressureStandard}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureStandard| is the standard atmospheric pressure in SI +% units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PressureStandard\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PressureStandard}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureStandard| is the standard atmospheric pressure in cgs +% units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PressureStandard\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PressureStandard}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureStandard| is the standard atmospheric pressure in cgs +% units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PressureStandard\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PressureStandard}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureStandardNumeric| is a mathematical value of +% the standard atmospheric pressure in SI units +% with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PressureStandardNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PressureStandardNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureStandardNumeric| is a mathematical value of +% the standard atmospheric pressure in SI units +% with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PressureStandardNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PressureStandardNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureStandardNumeric| is a mathematical value of +% the standard atmospheric pressure in cgs units +% with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PressureStandardNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PressureStandardNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureStandardNumeric| is a mathematical value of +% the standard atmospheric pressure in cgs units +% with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PressureStandardNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PressureStandardNumeric}\end{mdframed} +% \makeatother +% +% +%\subsubsection{Velocity, Speed and Acceleration} +% +% \DescribeMacro{\k@SI@short@SpeedLight} +% |\k@SI@short@SpeedLight| is the speed of light in SI units with reduced +% precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@SpeedLight\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@SpeedLight}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@SpeedLight} +% |\k@SI@full@SpeedLight| is the speed of light in SI units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@SpeedLight\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@SpeedLight}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@SpeedLight} +% |\k@cgs@short@SpeedLight| is the speed of light in cgs units with reduced +% precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@SpeedLight\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@SpeedLight}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@SpeedLight} +% |\k@cgs@full@SpeedLight| is the speed of light in cgs units with full +% precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@SpeedLight\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@SpeedLight}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@SpeedLightNumeric} +% |\k@SI@short@SpeedLightNumeric| is a mathematical value of +% the speed of light in SI units with reduced precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@SpeedLightNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@SpeedLightNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@SpeedLightNumeric} +% |\k@SI@full@SpeedLightNumeric| is a mathematical value of +% the speed of light in SI units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@SpeedLightNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@SpeedLightNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@SpeedLightNumeric} +% |\k@cgs@short@SpeedLightNumeric| is a mathematical value of +% the speed of light in cgs units with reduced +% precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@SpeedLightNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@SpeedLightNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@SpeedLightNumeric} +% |\k@cgs@full@SpeedLightNumeric| is a mathematical value of +% the speed of light in cgs units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@SpeedLightNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@SpeedLightNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@short@AccelGravity| is the accelertion due to gravity at the surface +% of the Earth in SI units with reduced precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@AccelGravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@AccelGravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@full@AccelGravity| is the accelertion due to gravity at the surface of +% the Earth in SI units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@AccelGravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@AccelGravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@short@AccelGravity| is the accelertion due to gravity at the surface +% of the Earth in cgs units with reduced precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@AccelGravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@AccelGravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@full@AccelGravity| is the accelertion due to gravity at the surface +% of the Earth in cgs units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@AccelGravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@AccelGravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@short@AccelGravityNumeric| is a mathematical value of +% the accelertion due to gravity at the surface of the +% Earth in SI units with reduced precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@AccelGravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@AccelGravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@full@AccelGravityNumeric| is a mathematical value of +% the accelertion due to gravity at the surface of the +% Earth in SI units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@AccelGravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@AccelGravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@short@AccelGravityNumeric| is a mathematical value of +% the accelertion due to gravity at the surface of +% the Earth in cgs units with reduced precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@AccelGravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@AccelGravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@full@AccelGravityNumeric| is a mathematical value of +% the accelertion due to gravity at the surface of the +% Earth in cgs units with full precision. +% (CODATA 2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@AccelGravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@AccelGravityNumeric}\end{mdframed} +% \makeatother +% +% +%\subsubsection{Other Constants} +% +% \DescribeMacro{\k@SI@short@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% SI units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@Coulomb\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@Coulomb}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% SI units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@Coulomb\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@Coulomb}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) +% in cgs units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@Coulomb\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@Coulomb}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% cgs units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@Coulomb\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@Coulomb}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@CoulombNumeric| is a mathematical value of +% the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in SI +% units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@CoulombNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@CoulombNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@CoulombNumeric| is a mathematical value of +% the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in SI +% units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@CoulombNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@CoulombNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@CoulombNumeric| is a mathematical value of +% the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in cgs +% units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@CoulombNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@CoulombNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@CoulombNumeric| is a mathematical value of +% the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in cgs +% units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@CoulombNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@CoulombNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@VacuumPermittivity} +% |\k@SI@short@VacuumPermittivity| is the electric permittivity of the vacuum +% in SI units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@VacuumPermittivity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@VacuumPermittivity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@VacuumPermittivity} +% |\k@SI@full@VacuumPermittivity| is the electric permittivity of the vacuum in +% SI units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@VacuumPermittivity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@VacuumPermittivity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@VacuumPermittivity} +% |\k@cgs@short@VacuumPermittivity| is the electric permittivity of the vacuum +% in cgs units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@VacuumPermittivity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@VacuumPermittivity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@VacuumPermittivity} +% |\k@cgs@full@VacuumPermittivity| is the electric permittivity of the vacuum +% in cgs units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@VacuumPermittivity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@VacuumPermittivity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@VacuumPermittivityNumeric} +% |\k@SI@short@VacuumPermittivityNumeric| is a mathematical value of +% the electric permittivity of the vacuum in SI +% units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@VacuumPermittivityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@VacuumPermittivityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@VacuumPermittivityNumeric} +% |\k@SI@full@VacuumPermittivityNumeric| is a mathematical value of +% the electric permittivity of the vacuum in SI +% units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@VacuumPermittivityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@VacuumPermittivityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@VacuumPermittivityNumeric} +% |\k@cgs@short@VacuumPermittivityNumeric| is a mathematical value of +% the electric permittivity of the vacuum in +% cgs units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@VacuumPermittivityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@VacuumPermittivityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@VacuumPermittivityNumeric} +% |\k@cgs@full@VacuumPermittivityNumeric| is a mathematical value of +% the electric permittivity of the vacuum in cgs +% units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@VacuumPermittivityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@VacuumPermittivityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@VacuumPermeability| is the magnetic permeability of the vacuum +% in SI units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@VacuumPermeability\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@VacuumPermeability}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@VacuumPermeability| is the magnetic permeability of the vacuum in +% SI units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@VacuumPermeability\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@VacuumPermeability}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@VacuumPermeability| is the magnetic permeability of the vacuum +% in cgs units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@VacuumPermeability\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@VacuumPermeability}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@VacuumPermeability| is the magnetic permeability of the vacuum +% in cgs units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@VacuumPermeability\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@VacuumPermeability}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@VacuumPermeabilityNumeric| is a mathematical value of +% the magnetic permeability of the vacuum in SI +% units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@VacuumPermeabilityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@VacuumPermeabilityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@VacuumPermeabilityNumeric| is a mathematical value of +% the magnetic permeability of the vacuum in SI +% units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@VacuumPermeabilityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@VacuumPermeabilityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@VacuumPermeabilityNumeric| is a mathematical value of +% the magnetic permeability of the vacuum in +% cgs units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@VacuumPermeabilityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@VacuumPermeabilityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@VacuumPermeabilityNumeric| is a mathematical value of +% the magnetic permeability of the vacuum in cgs +% units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@VacuumPermeabilityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@VacuumPermeabilityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@VacuumImpedance} +% |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with +% reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@VacuumImpedance\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@VacuumImpedance}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@VacuumImpedance} +% |\k@full@VacuumImpedance| is the characteristic impedance of the vacuum with +% full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@VacuumImpedance\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@VacuumImpedance}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@VacuumImpedanceNumeric} +% |\k@short@VacuumImpedanceNumeric| is a mathematical value of +% the characteristic impedance of the vacuum with +% reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@VacuumImpedanceNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@VacuumImpedanceNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@VacuumImpedanceNumeric} +% |\k@full@VacuumImpedanceNumeric| is a mathematical value of +% the characteristic impedance of the vacuum with full +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@VacuumImpedanceNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@VacuumImpedanceNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@Boltzmann} +% |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@Boltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@Boltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@Boltzmann} +% |\k@SI@full@Boltzmann| is the Boltzmann constant in SI units with full +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@Boltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@Boltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@Boltzmann} +% |\k@cgs@short@Boltzmann| is the Boltzmann constant in cgs units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@Boltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@Boltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@Boltzmann} +% |\k@cgs@full@Boltzmann| is the Boltzmann constant in cgs units with full +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@Boltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@Boltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@short@Boltzmann} +% |\k@eV@short@Boltzmann| is the Boltzmann constant in eV with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@short@Boltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@Boltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@full@Boltzmann} +% |\k@eV@full@Boltzmann| is the Boltzmann constant in eV with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@full@Boltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@Boltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@BoltzmannNumeric} +% |\k@SI@short@BoltzmannNumeric| is a mathematical value of +% the Boltzmann constant in SI units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@BoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@BoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@BoltzmannNumeric} +% |\k@SI@full@BoltzmannNumeric| is a mathematical value of +% the Boltzmann constant in SI units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@BoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@BoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@BoltzmannNumeric} +% |\k@cgs@short@BoltzmannNumeric| is a mathematical value of +% the Boltzmann constant in cgs units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@BoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@BoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@BoltzmannNumeric} +% |\k@cgs@full@BoltzmannNumeric| is a mathematical value of +% the Boltzmann constant in cgs units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@BoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@BoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@short@BoltzmannNumeric} +% |\k@eV@short@BoltzmannNumeric| is a mathematical value of +% the Boltzmann constant in eV with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@short@BoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@BoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@full@BoltzmannNumeric} +% |\k@eV@full@BoltzmannNumeric| is a mathematical value of +% the Boltzmann constant in eV with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@full@BoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@BoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@Planck| is the Planck constant in SI units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@Planck\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@Planck}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@Planck| is the Planck constant in SI units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@Planck\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@Planck}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@Planck| is the Planck constant in cgs units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@Planck\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@Planck}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@Planck| is the Planck constant in cgs units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@Planck\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@Planck}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@short@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@Planck| is the Planck constant in eV with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@short@Planck\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@Planck}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@full@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@Planck| is the Planck constant in eV with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@full@Planck\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@Planck}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@PlanckNumeric| is a mathematical value of +% the Planck constant in SI units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PlanckNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PlanckNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@PlanckNumeric| is a mathematical value of +% the Planck constant in SI units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PlanckNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PlanckNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@PlanckNumeric| is a mathematical value of +% the Planck constant in cgs units with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PlanckNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PlanckNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@PlanckNumeric| is a mathematical value of +% the Planck constant in cgs units with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PlanckNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PlanckNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@short@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@PlanckNumeric| is a mathematical value of +% the Planck constant in eV with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@short@PlanckNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@PlanckNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@full@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@PlanckNumeric| is a mathematical value of +% the Planck constant in eV with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@full@PlanckNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@PlanckNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PlanckReduced\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PlanckReduced}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in SI units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PlanckReduced\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PlanckReduced}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PlanckReduced\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PlanckReduced}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PlanckReduced\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PlanckReduced}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@short@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@short@PlanckReduced\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@PlanckReduced}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@full@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in eV with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@full@PlanckReduced\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@PlanckReduced}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@PlanckReducedNumeric| is a mathematical value of +% the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@PlanckReducedNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@PlanckReducedNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@PlanckReducedNumeric| is a mathematical value of +% the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in SI units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@PlanckReducedNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@PlanckReducedNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@PlanckReducedNumeric| is a mathematical value of +% the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@PlanckReducedNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@PlanckReducedNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@PlanckReducedNumeric| is a mathematical value of +% the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@PlanckReducedNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@PlanckReducedNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@short@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@PlanckReducedNumeric| is a mathematical value of +% the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@short@PlanckReducedNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@PlanckReducedNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@eV@full@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@PlanckReducedNumeric| is a mathematical value of +% the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in eV with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@eV@full@PlanckReducedNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@PlanckReducedNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@Gravity| is Newton's gravitational constant in SI units with +% reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@Gravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@Gravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@Gravity| is Newton's gravitational constant in SI units with full +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@Gravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@Gravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@Gravity| is Newton's gravitational constant in cgs units with +% reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@Gravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@Gravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@Gravity| is Newton's gravitational constant in cgs units with +% full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@Gravity\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@Gravity}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@GravityNumeric| is a mathematical value of +% Newton's gravitational constant in SI units with reduced +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@GravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@GravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@GravityNumeric| is a mathematical value of +% Newton's gravitational constant in SI units with full +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@GravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@GravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@GravityNumeric| is a mathematical value of +% Newton's gravitational constant in cgs units with +% reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@GravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@GravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@GravityNumeric| is a mathematical value of +% Newton's gravitational constant in cgs units with full +% precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@GravityNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@GravityNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@StefanBoltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@StefanBoltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@StefanBoltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@StefanBoltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@StefanBoltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@StefanBoltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@StefanBoltzmann\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@StefanBoltzmann}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@StefanBoltzmannNumeric| is a mathematical value of +% the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@StefanBoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@StefanBoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@StefanBoltzmannNumeric| is a mathematical value of +% the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@StefanBoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@StefanBoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@StefanBoltzmannNumeric| is a mathematical value of +% the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@StefanBoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@StefanBoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@StefanBoltzmannNumeric| is a mathematical value of +% the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@StefanBoltzmannNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@StefanBoltzmannNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@Radiation} +% |\k@SI@short@Radiation| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@Radiation\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@Radiation}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@Radiation} +% |\k@SI@full@Radiation| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@Radiation\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@Radiation}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@Radiation} +% |\k@cgs@short@Radiation| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@Radiation\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@Radiation}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@Radiation} +% |\k@cgs@full@Radiation| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@Radiation\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@Radiation}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@short@RadiationNumeric} +% |\k@SI@short@RadiationNumeric| is a mathematical value of +% the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@RadiationNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@RadiationNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@SI@full@RadiationNumeric} +% |\k@SI@full@RadiationNumeric| is a mathematical value of +% the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@RadiationNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@RadiationNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@short@RadiationNumeric} +% |\k@cgs@short@RadiationNumeric| is a mathematical value of +% the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@short@RadiationNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@RadiationNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@cgs@full@RadiationNumeric} +% |\k@cgs@full@RadiationNumeric| is a mathematical value of +% the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with full +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@cgs@full@RadiationNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@RadiationNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@FineStructure} +% |\k@short@FineStructure| is the fine structure constant with reduced +% precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@FineStructure\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@FineStructure}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@FineStructure} +% |\k@full@FineStructure| is the fine structure constant with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@FineStructure\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@FineStructure}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@FineStructureNumeric} +% |\k@short@FineStructureNumeric| is a mathematical value of +% the fine structure constant with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@FineStructureNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@FineStructureNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@FineStructureNumeric} +% |\k@full@FineStructureNumeric| is a mathematical value of +% the fine structure constant with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@FineStructureNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@FineStructureNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@FineStructureReciprocal} +% |\k@short@FineStructureReciprocal| is the reciprocal of the fine structure +% constant with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@FineStructureReciprocal\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@FineStructureReciprocal}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@FineStructureReciprocal} +% |\k@full@FineStructureReciprocal| is the reciprocal of the fine structure +% constant with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@FineStructureReciprocal\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@FineStructureReciprocal}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@FineStructureReciprocalNumeric} +% |\k@short@FineStructureReciprocalNumeric| is a mathematical value of +% the reciprocal of the fine structure +% constant with reduced precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@FineStructureReciprocalNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@FineStructureReciprocalNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@FineStructureReciprocalNumeric} +% |\k@full@FineStructureReciprocalNumeric| is a mathematical value of +% the reciprocal of the fine structure constant +% with full precision. +% (Calculated) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@FineStructureReciprocalNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@FineStructureReciprocalNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@Avogadro} +% |\k@short@Avogadro| is Avogadro's Number (the number of particles in a mole) +% with reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@Avogadro\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@Avogadro}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@Avogadro} +% |\k@full@Avogadro| is Avogadro's Number (the number of particles in a mole) +% with full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@Avogadro\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@Avogadro}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@short@AvogadroNumeric} +% |\k@short@AvogadroNumeric| is a mathematical value of +% Avogadro's Number (the number of particles in a mole) with +% reduced precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@short@AvogadroNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@AvogadroNumeric}\end{mdframed} +% \makeatother +% +% \DescribeMacro{\k@full@AvogadroNumeric} +% |\k@full@AvogadroNumeric| is a mathematical value of +% Avogadro's Number (the number of particles in a mole) with +% full precision. +% (CODATA~2018) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@full@AvogadroNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@AvogadroNumeric}\end{mdframed} +% \makeatother +% +\makeatletter +% \StopEventually{} +% +% \section{Implementation} +% +% \subsection{Special} +% +%\iffalse +%<*package> +%\fi +% \begin{macro}{\physconst@decimalsseparator} +% |\physconst@decimalsseparator| is the a special macro used to separate digits +% in the decimal portion of the constants. If the option unseparatedecimals is +% not specified, decimals will be printed as 1.234\,567\,890. If the option +% is specified, decimals will be printed as 1.234567890. This macro should +% note be used outside of this package. +% +% \begin{macrocode} +\ifx\unseparatedecimals\undefined +\DeclareRobustCommand{\physconst@decimalsseparator}{\,} +\else +\DeclareRobustCommand{\physconst@decimalsseparator}{ } +\fi +% \end{macrocode} +% \end{macro} +%\iffalse +% +%\fi +% +%\subsection{Mass} +% +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassElectron| is the mass of an electron in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassElectron}{% +\ensuremath{% +9.11% +\times 10^{-31}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassElectron| is the mass of an electron in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassElectron}{% +\ensuremath{% +9.108\expandafter\physconst@decimalsseparator% +980\expandafter\physconst@decimalsseparator% +087\expandafter\physconst@decimalsseparator% +382% +\times 10^{-31}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassElectron| is the mass of an electron in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassElectron}{% +\ensuremath{% +9.11% +\times 10^{-28}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassElectron| is the mass of an electron in cgs units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassElectron}{% +\ensuremath{% +9.108\expandafter\physconst@decimalsseparator% +980\expandafter\physconst@decimalsseparator% +087\expandafter\physconst@decimalsseparator% +382% +\times 10^{-28}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassElectron| is the mass of an electron in eV with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassElectron}{% +\ensuremath{% +5.11% +\times 10^{5}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassElectron| is the mass of an electron in eV with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassElectron}{% +\ensuremath{% +5.109\expandafter\physconst@decimalsseparator% +763\expandafter\physconst@decimalsseparator% +089\expandafter\physconst@decimalsseparator% +046% +\times 10^{5}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassElectron| is the mass of an electron. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassElectron}{% +\k@SI@short@MassElectron} +\else +\DeclareRobustCommand {\kMassElectron}{% +\k@SI@full@MassElectron} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassElectron}{% +\k@cgs@short@MassElectron} +\else +\DeclareRobustCommand {\kMassElectron}{% +\k@cgs@full@MassElectron} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassElectron} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassElectron| is the mass of an electron. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassElectron}{% +\k@eV@short@MassElectron} +\else +\DeclareRobustCommand {\keVMassElectron}{% +\k@eV@full@MassElectron} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassElectronNumeric| is the mass of an electron in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassElectronNumeric}{% +\ensuremath{% +9.11e-31}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassElectronNumeric| is the mass of an electron in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassElectronNumeric}{% +\ensuremath{% +9.108980087382e-31}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassElectronNumeric| is the mass of an electron in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassElectronNumeric}{% +\ensuremath{% +9.11e-28}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassElectronNumeric| is the mass of an electron in cgs units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassElectronNumeric}{% +\ensuremath{% +9.108980087382e-28}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassElectronNumeric| is the mass of an electron in eV with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassElectronNumeric}{% +\ensuremath{% +5.11e+05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassElectronNumeric| is the mass of an electron in eV with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassElectronNumeric}{% +\ensuremath{% +5.109763089046e+05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassElectronNumeric| is the mass of an electron. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassElectronNumeric}{% +\k@SI@short@MassElectronNumeric} +\else +\DeclareRobustCommand {\kMassElectronNumeric}{% +\k@SI@full@MassElectronNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassElectronNumeric}{% +\k@cgs@short@MassElectronNumeric} +\else +\DeclareRobustCommand {\kMassElectronNumeric}{% +\k@cgs@full@MassElectronNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassElectronNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassElectronNumeric| is the mass of an electron. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassElectronNumeric}{% +\k@eV@short@MassElectronNumeric} +\else +\DeclareRobustCommand {\keVMassElectronNumeric}{% +\k@eV@full@MassElectronNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassProton| is the mass of a proton in SI units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassProton}{% +\ensuremath{% +1.67% +\times 10^{-27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassProton| is the mass of a proton in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassProton}{% +\ensuremath{% +1.672\expandafter\physconst@decimalsseparator% +547\expandafter\physconst@decimalsseparator% +813\expandafter\physconst@decimalsseparator% +969% +\times 10^{-27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassProton| is the mass of a proton in cgs units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassProton}{% +\ensuremath{% +1.67% +\times 10^{-24}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassProton| is the mass of a proton in cgs units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassProton}{% +\ensuremath{% +1.672\expandafter\physconst@decimalsseparator% +547\expandafter\physconst@decimalsseparator% +813\expandafter\physconst@decimalsseparator% +969% +\times 10^{-24}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassProton| is the mass of a proton in eV with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassProton}{% +\ensuremath{% +9.38% +\times 10^{8}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassProton| is the mass of a proton in eV with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassProton}{% +\ensuremath{% +9.382\expandafter\physconst@decimalsseparator% +305\expandafter\physconst@decimalsseparator% +156\expandafter\physconst@decimalsseparator% +558% +\times 10^{8}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassProton| is the mass of a proton. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassProton}{% +\k@SI@short@MassProton} +\else +\DeclareRobustCommand {\kMassProton}{% +\k@SI@full@MassProton} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassProton}{% +\k@cgs@short@MassProton} +\else +\DeclareRobustCommand {\kMassProton}{% +\k@cgs@full@MassProton} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassProton} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassProton| is the mass of a proton. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassProton}{% +\k@eV@short@MassProton} +\else +\DeclareRobustCommand {\keVMassProton}{% +\k@eV@full@MassProton} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassProtonNumeric| is the mass of a proton in SI units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassProtonNumeric}{% +\ensuremath{% +1.67e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassProtonNumeric| is the mass of a proton in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassProtonNumeric}{% +\ensuremath{% +1.672547813969e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassProtonNumeric| is the mass of a proton in cgs units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassProtonNumeric}{% +\ensuremath{% +1.67e-24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassProtonNumeric| is the mass of a proton in cgs units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassProtonNumeric}{% +\ensuremath{% +1.672547813969e-24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassProtonNumeric| is the mass of a proton in eV with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassProtonNumeric}{% +\ensuremath{% +9.38e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassProtonNumeric| is the mass of a proton in eV with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassProtonNumeric}{% +\ensuremath{% +9.382305156558e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassProtonNumeric| is the mass of a proton. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassProtonNumeric}{% +\k@SI@short@MassProtonNumeric} +\else +\DeclareRobustCommand {\kMassProtonNumeric}{% +\k@SI@full@MassProtonNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassProtonNumeric}{% +\k@cgs@short@MassProtonNumeric} +\else +\DeclareRobustCommand {\kMassProtonNumeric}{% +\k@cgs@full@MassProtonNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassProtonNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassProtonNumeric| is the mass of a proton. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassProtonNumeric}{% +\k@eV@short@MassProtonNumeric} +\else +\DeclareRobustCommand {\keVMassProtonNumeric}{% +\k@eV@full@MassProtonNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassHydrogen| is the mass of a neutral hydrogen atom in SI units +% with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassHydrogen}{% +\ensuremath{% +1.67% +\times 10^{-27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassHydrogen| is the mass of a neutral hydrogen atom in SI units +% with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassHydrogen}{% +\ensuremath{% +1.673\expandafter\physconst@decimalsseparator% +458\expandafter\physconst@decimalsseparator% +687\expandafter\physconst@decimalsseparator% +724% +\times 10^{-27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassHydrogen| is the mass of a neutral hydrogen atom in cgs +% units with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassHydrogen}{% +\ensuremath{% +1.67% +\times 10^{-24}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassHydrogen| is the mass of a neutral hydrogen atom in cgs +% units with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassHydrogen}{% +\ensuremath{% +1.673\expandafter\physconst@decimalsseparator% +458\expandafter\physconst@decimalsseparator% +687\expandafter\physconst@decimalsseparator% +724% +\times 10^{-24}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassHydrogen| is the mass of a neutral hydrogen atom in eV with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassHydrogen}{% +\ensuremath{% +9.39% +\times 10^{8}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassHydrogen| is the mass of a neutral hydrogen atom in eV with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassHydrogen}{% +\ensuremath{% +9.387\expandafter\physconst@decimalsseparator% +414\expandafter\physconst@decimalsseparator% +783\expandafter\physconst@decimalsseparator% +596% +\times 10^{8}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassHydrogen| is the mass of a neutral hydrogen atom. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassHydrogen}{% +\k@SI@short@MassHydrogen} +\else +\DeclareRobustCommand {\kMassHydrogen}{% +\k@SI@full@MassHydrogen} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassHydrogen}{% +\k@cgs@short@MassHydrogen} +\else +\DeclareRobustCommand {\kMassHydrogen}{% +\k@cgs@full@MassHydrogen} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassHydrogen} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassHydrogen| is the mass of a neutral hydrogen atom. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassHydrogen}{% +\k@eV@short@MassHydrogen} +\else +\DeclareRobustCommand {\keVMassHydrogen}{% +\k@eV@full@MassHydrogen} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in SI units +% with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassHydrogenNumeric}{% +\ensuremath{% +1.67e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in SI units +% with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassHydrogenNumeric}{% +\ensuremath{% +1.673458687724e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in cgs +% units with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassHydrogenNumeric}{% +\ensuremath{% +1.67e-24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in cgs +% units with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassHydrogenNumeric}{% +\ensuremath{% +1.673458687724e-24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in eV with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassHydrogenNumeric}{% +\ensuremath{% +9.39e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassHydrogenNumeric| is the mass of a neutral hydrogen atom in eV with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassHydrogenNumeric}{% +\ensuremath{% +9.387414783596e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassHydrogenNumeric| is the mass of a neutral hydrogen atom. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassHydrogenNumeric}{% +\k@SI@short@MassHydrogenNumeric} +\else +\DeclareRobustCommand {\kMassHydrogenNumeric}{% +\k@SI@full@MassHydrogenNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassHydrogenNumeric}{% +\k@cgs@short@MassHydrogenNumeric} +\else +\DeclareRobustCommand {\kMassHydrogenNumeric}{% +\k@cgs@full@MassHydrogenNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassHydrogenNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassHydrogenNumeric| is the mass of a neutral hydrogen atom. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassHydrogenNumeric}{% +\k@eV@short@MassHydrogenNumeric} +\else +\DeclareRobustCommand {\keVMassHydrogenNumeric}{% +\k@eV@full@MassHydrogenNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassSun} +% |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassSun}{% +\ensuremath{% +1.99% +\times 10^{30}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassSun} +% |\k@SI@full@MassSun| is the mass of the Sun in SI units with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassSun}{% +\ensuremath{% +1.988\expandafter\physconst@decimalsseparator% +409\expandafter\physconst@decimalsseparator% +9% +\times 10^{30}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassSun} +% |\k@cgs@short@MassSun| is the mass of the Sun in cgs units with reduced +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassSun}{% +\ensuremath{% +1.99% +\times 10^{33}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassSun} +% |\k@cgs@full@MassSun| is the mass of the Sun in cgs units with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassSun}{% +\ensuremath{% +1.988\expandafter\physconst@decimalsseparator% +409\expandafter\physconst@decimalsseparator% +9% +\times 10^{33}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassSun} +% |\kMassSun| is the mass of the Sun. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassSun}{% +\k@SI@short@MassSun} +\else +\DeclareRobustCommand {\kMassSun}{% +\k@SI@full@MassSun} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassSun}{% +\k@cgs@short@MassSun} +\else +\DeclareRobustCommand {\kMassSun}{% +\k@cgs@full@MassSun} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassSunNumeric} +% |\k@SI@short@MassSunNumeric| is the mass of the Sun in SI units with reduced +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassSunNumeric}{% +\ensuremath{% +1.99e+30}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassSunNumeric} +% |\k@SI@full@MassSunNumeric| is the mass of the Sun in SI units with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassSunNumeric}{% +\ensuremath{% +1.9884099e+30}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassSunNumeric} +% |\k@cgs@short@MassSunNumeric| is the mass of the Sun in cgs units with reduced +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassSunNumeric}{% +\ensuremath{% +1.99e+33}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassSunNumeric} +% |\k@cgs@full@MassSunNumeric| is the mass of the Sun in cgs units with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassSunNumeric}{% +\ensuremath{% +1.9884099e+33}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassSunNumeric} +% |\kMassSunNumeric| is the mass of the Sun. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassSunNumeric}{% +\k@SI@short@MassSunNumeric} +\else +\DeclareRobustCommand {\kMassSunNumeric}{% +\k@SI@full@MassSunNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassSunNumeric}{% +\k@cgs@short@MassSunNumeric} +\else +\DeclareRobustCommand {\kMassSunNumeric}{% +\k@cgs@full@MassSunNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@MassEarth} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@short@MassEarth| is the mass of the Earth with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@MassEarth}{% +\ensuremath{% +5.97% +\times 10^{24}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@MassEarth} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@full@MassEarth| is the mass of the Earth with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@MassEarth}{% +\ensuremath{% +5.972\expandafter\physconst@decimalsseparator% +168% +\times 10^{24}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassEarth} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\kMassEarth| is the mass of the Earth. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassEarth}{% +\k@short@MassEarth} +\else +\DeclareRobustCommand {\kMassEarth}{% +\k@full@MassEarth} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@MassEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@short@MassEarthNumeric| is the mass of the Earth with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@MassEarthNumeric}{% +\ensuremath{% +5.97e+24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@MassEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\k@full@MassEarthNumeric| is the mass of the Earth with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@MassEarthNumeric}{% +\ensuremath{% +5.972168e+24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Earth} +% |\kMassEarthNumeric| is the mass of the Earth. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassEarthNumeric}{% +\k@short@MassEarthNumeric} +\else +\DeclareRobustCommand {\kMassEarthNumeric}{% +\k@full@MassEarthNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@MassJupiter} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@short@MassJupiter| is the mass of Jupiter with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@MassJupiter}{% +\ensuremath{% +1.90% +\times 10^{27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@MassJupiter} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@full@MassJupiter| is the mass of Jupiter with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@MassJupiter}{% +\ensuremath{% +1.898\expandafter\physconst@decimalsseparator% +124\expandafter\physconst@decimalsseparator% +6% +\times 10^{27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassJupiter} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\kMassJupiter| is the mass of Jupiter. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassJupiter}{% +\k@short@MassJupiter} +\else +\DeclareRobustCommand {\kMassJupiter}{% +\k@full@MassJupiter} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@MassJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@short@MassJupiterNumeric| is the mass of Jupiter with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@MassJupiterNumeric}{% +\ensuremath{% +1.90e+27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@MassJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\k@full@MassJupiterNumeric| is the mass of Jupiter with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@MassJupiterNumeric}{% +\ensuremath{% +1.8981246e+27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add mass of Jupiter} +% |\kMassJupiterNumeric| is the mass of Jupiter. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassJupiterNumeric}{% +\k@short@MassJupiterNumeric} +\else +\DeclareRobustCommand {\kMassJupiterNumeric}{% +\k@full@MassJupiterNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassAMU| is the mass of an atomic mass unit in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassAMU}{% +\ensuremath{% +1.66% +\times 10^{-27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassAMU| is the mass of an atomic mass unit in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassAMU}{% +\ensuremath{% +1.660\expandafter\physconst@decimalsseparator% +465\expandafter\physconst@decimalsseparator% +492\expandafter\physconst@decimalsseparator% +239% +\times 10^{-27}\kg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassAMU| is the mass of an atomic mass unit in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassAMU}{% +\ensuremath{% +1.66% +\times 10^{-24}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassAMU| is the mass of an atomic mass unit in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassAMU}{% +\ensuremath{% +1.660\expandafter\physconst@decimalsseparator% +465\expandafter\physconst@decimalsseparator% +492\expandafter\physconst@decimalsseparator% +239% +\times 10^{-24}\gm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassAMU| is the mass of an atomic mass unit in eV with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassAMU}{% +\ensuremath{% +9.31% +\times 10^{8}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassAMU| is the mass of an atomic mass unit in eV with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassAMU}{% +\ensuremath{% +9.314\expandafter\physconst@decimalsseparator% +528\expandafter\physconst@decimalsseparator% +302\expandafter\physconst@decimalsseparator% +276% +\times 10^{8}\eV\,c^{-2}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassAMU| is the mass of an atomic mass unit. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassAMU}{% +\k@SI@short@MassAMU} +\else +\DeclareRobustCommand {\kMassAMU}{% +\k@SI@full@MassAMU} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassAMU}{% +\k@cgs@short@MassAMU} +\else +\DeclareRobustCommand {\kMassAMU}{% +\k@cgs@full@MassAMU} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassAMU} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassAMU| is the mass of an atomic mass unit. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassAMU}{% +\k@eV@short@MassAMU} +\else +\DeclareRobustCommand {\keVMassAMU}{% +\k@eV@full@MassAMU} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@short@MassAMUNumeric| is the mass of an atomic mass unit in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@MassAMUNumeric}{% +\ensuremath{% +1.66e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@SI@full@MassAMUNumeric| is the mass of an atomic mass unit in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@MassAMUNumeric}{% +\ensuremath{% +1.660465492239e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@short@MassAMUNumeric| is the mass of an atomic mass unit in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@MassAMUNumeric}{% +\ensuremath{% +1.66e-24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@cgs@full@MassAMUNumeric| is the mass of an atomic mass unit in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@MassAMUNumeric}{% +\ensuremath{% +1.660465492239e-24}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@short@MassAMUNumeric| is the mass of an atomic mass unit in eV with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@MassAMUNumeric}{% +\ensuremath{% +9.31e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@full@MassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\k@eV@full@MassAMUNumeric| is the mass of an atomic mass unit in eV with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@full@MassAMUNumeric}{% +\ensuremath{% +9.314528302276e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kMassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\kMassAMUNumeric| is the mass of an atomic mass unit. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassAMUNumeric}{% +\k@SI@short@MassAMUNumeric} +\else +\DeclareRobustCommand {\kMassAMUNumeric}{% +\k@SI@full@MassAMUNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kMassAMUNumeric}{% +\k@cgs@short@MassAMUNumeric} +\else +\DeclareRobustCommand {\kMassAMUNumeric}{% +\k@cgs@full@MassAMUNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVMassAMUNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% \changes{v1.1.0}{2020/02/03}{Correct value in eV.} +% |\keVMassAMUNumeric| is the mass of an atomic mass unit. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVMassAMUNumeric}{% +\k@eV@short@MassAMUNumeric} +\else +\DeclareRobustCommand {\keVMassAMUNumeric}{% +\k@eV@full@MassAMUNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +% +%\subsection{Charge} +% +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ChargeFundamental} +% |\k@SI@short@ChargeFundamental| is the fundamental charge in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ChargeFundamental}{% +\ensuremath{% +1.60% +\times 10^{-19}\Coulomb}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ChargeFundamental} +% |\k@SI@full@ChargeFundamental| is the fundamental charge in SI units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ChargeFundamental}{% +\ensuremath{% +1.602\expandafter\physconst@decimalsseparator% +176\expandafter\physconst@decimalsseparator% +634% +\times 10^{-19}\Coulomb}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ChargeFundamental} +% |\k@cgs@short@ChargeFundamental| is the fundamental charge in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ChargeFundamental}{% +\ensuremath{% +4.80% +\times 10^{-10}\esu}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ChargeFundamental} +% |\k@cgs@full@ChargeFundamental| is the fundamental charge in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ChargeFundamental}{% +\ensuremath{% +4.803\expandafter\physconst@decimalsseparator% +204\expandafter\physconst@decimalsseparator% +713% +\times 10^{-10}\esu}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kChargeFundamental} +% |\kChargeFundamental| is the fundamental charge. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeFundamental}{% +\k@SI@short@ChargeFundamental} +\else +\DeclareRobustCommand {\kChargeFundamental}{% +\k@SI@full@ChargeFundamental} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeFundamental}{% +\k@cgs@short@ChargeFundamental} +\else +\DeclareRobustCommand {\kChargeFundamental}{% +\k@cgs@full@ChargeFundamental} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ChargeFundamentalNumeric} +% |\k@SI@short@ChargeFundamentalNumeric| is the fundamental charge in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ChargeFundamentalNumeric}{% +\ensuremath{% +1.60e-19}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ChargeFundamentalNumeric} +% |\k@SI@full@ChargeFundamentalNumeric| is the fundamental charge in SI units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ChargeFundamentalNumeric}{% +\ensuremath{% +1.602176634e-19}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ChargeFundamentalNumeric} +% |\k@cgs@short@ChargeFundamentalNumeric| is the fundamental charge in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ChargeFundamentalNumeric}{% +\ensuremath{% +4.80e-10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ChargeFundamentalNumeric} +% |\k@cgs@full@ChargeFundamentalNumeric| is the fundamental charge in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ChargeFundamentalNumeric}{% +\ensuremath{% +4.803204713e-10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kChargeFundamentalNumeric} +% |\kChargeFundamentalNumeric| is the fundamental charge. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeFundamentalNumeric}{% +\k@SI@short@ChargeFundamentalNumeric} +\else +\DeclareRobustCommand {\kChargeFundamentalNumeric}{% +\k@SI@full@ChargeFundamentalNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeFundamentalNumeric}{% +\k@cgs@short@ChargeFundamentalNumeric} +\else +\DeclareRobustCommand {\kChargeFundamentalNumeric}{% +\k@cgs@full@ChargeFundamentalNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ChargeElectron} +% |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ChargeElectron}{% +\ensuremath{% +-1.60% +\times 10^{-19}\Coulomb}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ChargeElectron} +% |\k@SI@full@ChargeElectron| is the charge of an electron in SI units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ChargeElectron}{% +\ensuremath{% +-1.602\expandafter\physconst@decimalsseparator% +176\expandafter\physconst@decimalsseparator% +634% +\times 10^{-19}\Coulomb}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ChargeElectron} +% |\k@cgs@short@ChargeElectron| is the charge of an electron in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ChargeElectron}{% +\ensuremath{% +-4.80% +\times 10^{-10}\esu}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ChargeElectron} +% |\k@cgs@full@ChargeElectron| is the charge of an electron in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ChargeElectron}{% +\ensuremath{% +-4.803\expandafter\physconst@decimalsseparator% +204\expandafter\physconst@decimalsseparator% +713% +\times 10^{-10}\esu}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kChargeElectron} +% |\kChargeElectron| is the charge of an electron. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeElectron}{% +\k@SI@short@ChargeElectron} +\else +\DeclareRobustCommand {\kChargeElectron}{% +\k@SI@full@ChargeElectron} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeElectron}{% +\k@cgs@short@ChargeElectron} +\else +\DeclareRobustCommand {\kChargeElectron}{% +\k@cgs@full@ChargeElectron} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ChargeElectronNumeric} +% |\k@SI@short@ChargeElectronNumeric| is the charge of an electron in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ChargeElectronNumeric}{% +\ensuremath{% +-1.60e-19}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ChargeElectronNumeric} +% |\k@SI@full@ChargeElectronNumeric| is the charge of an electron in SI units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ChargeElectronNumeric}{% +\ensuremath{% +-1.602176634e-19}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ChargeElectronNumeric} +% |\k@cgs@short@ChargeElectronNumeric| is the charge of an electron in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ChargeElectronNumeric}{% +\ensuremath{% +-4.80e-10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ChargeElectronNumeric} +% |\k@cgs@full@ChargeElectronNumeric| is the charge of an electron in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ChargeElectronNumeric}{% +\ensuremath{% +-4.803204713e-10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kChargeElectronNumeric} +% |\kChargeElectronNumeric| is the charge of an electron. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeElectronNumeric}{% +\k@SI@short@ChargeElectronNumeric} +\else +\DeclareRobustCommand {\kChargeElectronNumeric}{% +\k@SI@full@ChargeElectronNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeElectronNumeric}{% +\k@cgs@short@ChargeElectronNumeric} +\else +\DeclareRobustCommand {\kChargeElectronNumeric}{% +\k@cgs@full@ChargeElectronNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ChargeProton} +% |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ChargeProton}{% +\ensuremath{% +1.60% +\times 10^{-19}\Coulomb}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ChargeProton} +% |\k@SI@full@ChargeProton| is the charge of a proton in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ChargeProton}{% +\ensuremath{% +1.602\expandafter\physconst@decimalsseparator% +176\expandafter\physconst@decimalsseparator% +634% +\times 10^{-19}\Coulomb}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ChargeProton} +% |\k@cgs@short@ChargeProton| is the charge of a proton in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ChargeProton}{% +\ensuremath{% +4.80% +\times 10^{-10}\esu}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ChargeProton} +% |\k@cgs@full@ChargeProton| is the charge of a proton in cgs units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ChargeProton}{% +\ensuremath{% +4.803\expandafter\physconst@decimalsseparator% +204\expandafter\physconst@decimalsseparator% +713% +\times 10^{-10}\esu}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kChargeProton} +% |\kChargeProton| is the charge of a proton. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeProton}{% +\k@SI@short@ChargeProton} +\else +\DeclareRobustCommand {\kChargeProton}{% +\k@SI@full@ChargeProton} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeProton}{% +\k@cgs@short@ChargeProton} +\else +\DeclareRobustCommand {\kChargeProton}{% +\k@cgs@full@ChargeProton} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ChargeProtonNumeric} +% |\k@SI@short@ChargeProtonNumeric| is the charge of a proton in SI units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ChargeProtonNumeric}{% +\ensuremath{% +1.60e-19}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ChargeProtonNumeric} +% |\k@SI@full@ChargeProtonNumeric| is the charge of a proton in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ChargeProtonNumeric}{% +\ensuremath{% +1.602176634e-19}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ChargeProtonNumeric} +% |\k@cgs@short@ChargeProtonNumeric| is the charge of a proton in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ChargeProtonNumeric}{% +\ensuremath{% +4.80e-10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ChargeProtonNumeric} +% |\k@cgs@full@ChargeProtonNumeric| is the charge of a proton in cgs units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ChargeProtonNumeric}{% +\ensuremath{% +4.803204713e-10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kChargeProtonNumeric} +% |\kChargeProtonNumeric| is the charge of a proton. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeProtonNumeric}{% +\k@SI@short@ChargeProtonNumeric} +\else +\DeclareRobustCommand {\kChargeProtonNumeric}{% +\k@SI@full@ChargeProtonNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kChargeProtonNumeric}{% +\k@cgs@short@ChargeProtonNumeric} +\else +\DeclareRobustCommand {\kChargeProtonNumeric}{% +\k@cgs@full@ChargeProtonNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +% +%\subsection{Distances and Lengths} +% +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@RadiusBohr} +% |\k@SI@short@RadiusBohr| is Bohr radius of an atom in SI units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@RadiusBohr}{% +\ensuremath{% +5.29% +\times 10^{-11}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@RadiusBohr} +% |\k@SI@full@RadiusBohr| is Bohr radius of an atom in SI units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@RadiusBohr}{% +\ensuremath{% +5.292\expandafter\physconst@decimalsseparator% +006\expandafter\physconst@decimalsseparator% +59% +\times 10^{-11}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@RadiusBohr} +% |\k@cgs@short@RadiusBohr| is Bohr radius of an atom in cgs units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@RadiusBohr}{% +\ensuremath{% +5.29% +\times 10^{-9}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@RadiusBohr} +% |\k@cgs@full@RadiusBohr| is Bohr radius of an atom in cgs units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@RadiusBohr}{% +\ensuremath{% +5.292\expandafter\physconst@decimalsseparator% +006\expandafter\physconst@decimalsseparator% +59% +\times 10^{-9}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusBohr} +% |\kRadiusBohr| is Bohr radius of an atom. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusBohr}{% +\k@SI@short@RadiusBohr} +\else +\DeclareRobustCommand {\kRadiusBohr}{% +\k@SI@full@RadiusBohr} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusBohr}{% +\k@cgs@short@RadiusBohr} +\else +\DeclareRobustCommand {\kRadiusBohr}{% +\k@cgs@full@RadiusBohr} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@RadiusBohrNumeric} +% |\k@SI@short@RadiusBohrNumeric| is Bohr radius of an atom in SI units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@RadiusBohrNumeric}{% +\ensuremath{% +5.29e-11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@RadiusBohrNumeric} +% |\k@SI@full@RadiusBohrNumeric| is Bohr radius of an atom in SI units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@RadiusBohrNumeric}{% +\ensuremath{% +5.29200659e-11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@RadiusBohrNumeric} +% |\k@cgs@short@RadiusBohrNumeric| is Bohr radius of an atom in cgs units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@RadiusBohrNumeric}{% +\ensuremath{% +5.29e-09}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@RadiusBohrNumeric} +% |\k@cgs@full@RadiusBohrNumeric| is Bohr radius of an atom in cgs units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@RadiusBohrNumeric}{% +\ensuremath{% +5.29200659e-09}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusBohrNumeric} +% |\kRadiusBohrNumeric| is Bohr radius of an atom. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusBohrNumeric}{% +\k@SI@short@RadiusBohrNumeric} +\else +\DeclareRobustCommand {\kRadiusBohrNumeric}{% +\k@SI@full@RadiusBohrNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusBohrNumeric}{% +\k@cgs@short@RadiusBohrNumeric} +\else +\DeclareRobustCommand {\kRadiusBohrNumeric}{% +\k@cgs@full@RadiusBohrNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@AstronomicalUnit} +% |\k@SI@short@AstronomicalUnit| is the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with reduced precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@AstronomicalUnit}{% +\ensuremath{% +1.50% +\times 10^{11}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@AstronomicalUnit} +% |\k@SI@full@AstronomicalUnit| is the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with full precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@AstronomicalUnit}{% +\ensuremath{% +1.495\expandafter\physconst@decimalsseparator% +978\expandafter\physconst@decimalsseparator% +707% +\times 10^{11}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@AstronomicalUnit} +% |\k@cgs@short@AstronomicalUnit| is the astronomical unit (the average +% distance between the Earth and the Sun) in cgs units with reduced precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@AstronomicalUnit}{% +\ensuremath{% +1.50% +\times 10^{13}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@AstronomicalUnit} +% |\k@cgs@full@AstronomicalUnit| is the astronomical unit (the average distance +% between the Earth and the Sun) in cgs units with full precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@AstronomicalUnit}{% +\ensuremath{% +1.495\expandafter\physconst@decimalsseparator% +978\expandafter\physconst@decimalsseparator% +707% +\times 10^{13}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kAstronomicalUnit} +% |\kAstronomicalUnit| is the astronomical unit (the average distance between +% the Earth and the Sun). +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kAstronomicalUnit}{% +\k@SI@short@AstronomicalUnit} +\else +\DeclareRobustCommand {\kAstronomicalUnit}{% +\k@SI@full@AstronomicalUnit} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kAstronomicalUnit}{% +\k@cgs@short@AstronomicalUnit} +\else +\DeclareRobustCommand {\kAstronomicalUnit}{% +\k@cgs@full@AstronomicalUnit} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@AstronomicalUnitNumeric} +% |\k@SI@short@AstronomicalUnitNumeric| is the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with reduced precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@AstronomicalUnitNumeric}{% +\ensuremath{% +1.50e+11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@AstronomicalUnitNumeric} +% |\k@SI@full@AstronomicalUnitNumeric| is the astronomical unit (the average distance +% between the Earth and the Sun) in SI units with full precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@AstronomicalUnitNumeric}{% +\ensuremath{% +1.495978707e+11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@AstronomicalUnitNumeric} +% |\k@cgs@short@AstronomicalUnitNumeric| is the astronomical unit (the average +% distance between the Earth and the Sun) in cgs units with reduced precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@AstronomicalUnitNumeric}{% +\ensuremath{% +1.50e+13}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@AstronomicalUnitNumeric} +% |\k@cgs@full@AstronomicalUnitNumeric| is the astronomical unit (the average distance +% between the Earth and the Sun) in cgs units with full precision. +% Source: IAU~Resolution~B2~2012 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@AstronomicalUnitNumeric}{% +\ensuremath{% +1.495978707e+13}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kAstronomicalUnitNumeric} +% |\kAstronomicalUnitNumeric| is the astronomical unit (the average distance between +% the Earth and the Sun). +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kAstronomicalUnitNumeric}{% +\k@SI@short@AstronomicalUnitNumeric} +\else +\DeclareRobustCommand {\kAstronomicalUnitNumeric}{% +\k@SI@full@AstronomicalUnitNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kAstronomicalUnitNumeric}{% +\k@cgs@short@AstronomicalUnitNumeric} +\else +\DeclareRobustCommand {\kAstronomicalUnitNumeric}{% +\k@cgs@full@AstronomicalUnitNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@Parsec} +% |\k@SI@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% SI units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@Parsec}{% +\ensuremath{% +3.09% +\times 10^{16}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@Parsec} +% |\k@SI@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in SI +% units with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@Parsec}{% +\ensuremath{% +3.085\expandafter\physconst@decimalsseparator% +677\expandafter\physconst@decimalsseparator% +581% +\times 10^{16}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@Parsec} +% |\k@cgs@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% cgs units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@Parsec}{% +\ensuremath{% +3.09% +\times 10^{18}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@Parsec} +% |\k@cgs@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% cgs units with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@Parsec}{% +\ensuremath{% +3.085\expandafter\physconst@decimalsseparator% +677\expandafter\physconst@decimalsseparator% +581% +\times 10^{18}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kParsec} +% |\kParsec| is the length of a parsec ($\frac{648000\au}{\pi}$). +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kParsec}{% +\k@SI@short@Parsec} +\else +\DeclareRobustCommand {\kParsec}{% +\k@SI@full@Parsec} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kParsec}{% +\k@cgs@short@Parsec} +\else +\DeclareRobustCommand {\kParsec}{% +\k@cgs@full@Parsec} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@ParsecNumeric} +% |\k@SI@short@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% SI units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@ParsecNumeric}{% +\ensuremath{% +3.09e+16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@ParsecNumeric} +% |\k@SI@full@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in SI +% units with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@ParsecNumeric}{% +\ensuremath{% +3.085677581e+16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@ParsecNumeric} +% |\k@cgs@short@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% cgs units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@ParsecNumeric}{% +\ensuremath{% +3.09e+18}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@ParsecNumeric} +% |\k@cgs@full@ParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% cgs units with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@ParsecNumeric}{% +\ensuremath{% +3.085677581e+18}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kParsecNumeric} +% |\kParsecNumeric| is the length of a parsec ($\frac{648000\au}{\pi}$). +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kParsecNumeric}{% +\k@SI@short@ParsecNumeric} +\else +\DeclareRobustCommand {\kParsecNumeric}{% +\k@SI@full@ParsecNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kParsecNumeric}{% +\k@cgs@short@ParsecNumeric} +\else +\DeclareRobustCommand {\kParsecNumeric}{% +\k@cgs@full@ParsecNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@RadiusSun} +% |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@RadiusSun}{% +\ensuremath{% +6.96% +\times 10^{8}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@RadiusSun} +% |\k@SI@full@RadiusSun| is the mean radius of the Sun in SI units with full +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@RadiusSun}{% +\ensuremath{% +6.957% +\times 10^{8}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@RadiusSun} +% |\k@cgs@short@RadiusSun| is the mean radius of the Sun in cgs units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@RadiusSun}{% +\ensuremath{% +6.96% +\times 10^{10}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@RadiusSun} +% |\k@cgs@full@RadiusSun| is the mean radius of the Sun in cgs units with full +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@RadiusSun}{% +\ensuremath{% +6.957% +\times 10^{10}\cm}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusSun} +% |\kRadiusSun| is the mean radius of the Sun. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusSun}{% +\k@SI@short@RadiusSun} +\else +\DeclareRobustCommand {\kRadiusSun}{% +\k@SI@full@RadiusSun} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusSun}{% +\k@cgs@short@RadiusSun} +\else +\DeclareRobustCommand {\kRadiusSun}{% +\k@cgs@full@RadiusSun} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@RadiusSunNumeric} +% |\k@SI@short@RadiusSunNumeric| is the mean radius of the Sun in SI units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@RadiusSunNumeric}{% +\ensuremath{% +6.96e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@RadiusSunNumeric} +% |\k@SI@full@RadiusSunNumeric| is the mean radius of the Sun in SI units with full +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@RadiusSunNumeric}{% +\ensuremath{% +6.957e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@RadiusSunNumeric} +% |\k@cgs@short@RadiusSunNumeric| is the mean radius of the Sun in cgs units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@RadiusSunNumeric}{% +\ensuremath{% +6.96e+10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@RadiusSunNumeric} +% |\k@cgs@full@RadiusSunNumeric| is the mean radius of the Sun in cgs units with full +% precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@RadiusSunNumeric}{% +\ensuremath{% +6.957e+10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusSunNumeric} +% |\kRadiusSunNumeric| is the mean radius of the Sun. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusSunNumeric}{% +\k@SI@short@RadiusSunNumeric} +\else +\DeclareRobustCommand {\kRadiusSunNumeric}{% +\k@SI@full@RadiusSunNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusSunNumeric}{% +\k@cgs@short@RadiusSunNumeric} +\else +\DeclareRobustCommand {\kRadiusSunNumeric}{% +\k@cgs@full@RadiusSunNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@RadiusEarth} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@short@RadiusEarth| is the mean radius of the Earth with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@RadiusEarth}{% +\ensuremath{% +6.37% +\times 10^{6}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@RadiusEarth} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@full@RadiusEarth| is the mean radius of the Earth with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@RadiusEarth}{% +\ensuremath{% +6.371\expandafter\physconst@decimalsseparator% +0% +\times 10^{6}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusEarth} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\kRadiusEarth| is the mean radius of the Earth. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusEarth}{% +\k@short@RadiusEarth} +\else +\DeclareRobustCommand {\kRadiusEarth}{% +\k@full@RadiusEarth} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@RadiusEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@short@RadiusEarthNumeric| is the mean radius of the Earth with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@RadiusEarthNumeric}{% +\ensuremath{% +6.37e+06}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@RadiusEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\k@full@RadiusEarthNumeric| is the mean radius of the Earth with full precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@RadiusEarthNumeric}{% +\ensuremath{% +6.3710e+06}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusEarthNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Earth} +% |\kRadiusEarthNumeric| is the mean radius of the Earth. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusEarthNumeric}{% +\k@short@RadiusEarthNumeric} +\else +\DeclareRobustCommand {\kRadiusEarthNumeric}{% +\k@full@RadiusEarthNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@RadiusJupiter} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@short@RadiusJupiter| is the mean radius of Jupiter with reduced precision. +% Source: IAU~Resolution~B3~2015 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@RadiusJupiter}{% +\ensuremath{% +6.99% +\times 10^{7}\m}} +% \end{macrocode} +% \end{macro} % %\iffalse +% +%\fi +%\iffalse %<*package> %\fi -% \begin{macro}{\physconst@decimalsseparator} -% |\physconst@decimalsseparator| is the a special macro used to separate digits -% in the decimal portion of the constants. If the option unseparatedecimals is -% not specified, decimals will be printed as 1.234\,567\,890. If the option -% is specified, decimals will be printed as 1.234567890. This macro should -% note be used outside of this package. +% \begin{macro}{\k@full@RadiusJupiter} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@full@RadiusJupiter| is the mean radius of Jupiter with full precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\ifx\unseparatedecimals\undefined -\DeclareRobustCommand{\physconst@decimalsseparator}{\,} +\DeclareRobustCommand{\k@full@RadiusJupiter}{% +\ensuremath{% +6.991\expandafter\physconst@decimalsseparator% +1% +\times 10^{7}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusJupiter} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\kRadiusJupiter| is the mean radius of Jupiter. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusJupiter}{% +\k@short@RadiusJupiter} \else -\DeclareRobustCommand{\physconst@decimalsseparator}{ } +\DeclareRobustCommand {\kRadiusJupiter}{% +\k@full@RadiusJupiter} \fi % \end{macrocode} % \end{macro} +% %\iffalse % %\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@RadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@short@RadiusJupiterNumeric| is the mean radius of Jupiter with reduced precision. +% Source: IAU~Resolution~B3~2015 % -%\subsection{Mass} +% \begin{macrocode} +\DeclareRobustCommand{\k@short@RadiusJupiterNumeric}{% +\ensuremath{% +6.99e+07}} +% \end{macrocode} +% \end{macro} % %\iffalse +% +%\fi +%\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@MassElectron} -% |\k@SI@short@MassElectron| is the mass of an electron in SI units with -% reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@full@RadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\k@full@RadiusJupiterNumeric| is the mean radius of Jupiter with full precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@MassElectron}{% +\DeclareRobustCommand{\k@full@RadiusJupiterNumeric}{% \ensuremath{% -9.11% -\times 10^{-34}\kg}} +6.9911e+07}} % \end{macrocode} % \end{macro} % @@ -2545,19 +9081,40 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@MassElectron} -% |\k@SI@full@MassElectron| is the mass of an electron in SI units with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\kRadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\kRadiusJupiterNumeric| is the mean radius of Jupiter. % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@MassElectron}{% +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusJupiterNumeric}{% +\k@short@RadiusJupiterNumeric} +\else +\DeclareRobustCommand {\kRadiusJupiterNumeric}{% +\k@full@RadiusJupiterNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +% +%\subsection{Energy, Power, and Luminosity} +% +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@Rydberg} +% |\k@SI@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in SI units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@Rydberg}{% \ensuremath{% -9.108\expandafter\physconst@decimalsseparator% -980\expandafter\physconst@decimalsseparator% -087\expandafter\physconst@decimalsseparator% -382% -\times 10^{-34}\kg}} +2.18% +\times 10^{-18}\Joule}} % \end{macrocode} % \end{macro} % @@ -2567,16 +9124,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@MassElectron} -% |\k@cgs@short@MassElectron| is the mass of an electron in cgs units with -% reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@Rydberg} +% |\k@SI@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in SI units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@MassElectron}{% +\DeclareRobustCommand{\k@SI@full@Rydberg}{% \ensuremath{% -9.11% -\times 10^{-31}\gm}} +2.179\expandafter\physconst@decimalsseparator% +775\expandafter\physconst@decimalsseparator% +77% +\times 10^{-18}\Joule}} % \end{macrocode} % \end{macro} % @@ -2586,19 +9145,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@MassElectron} -% |\k@cgs@full@MassElectron| is the mass of an electron in cgs units with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@Rydberg} +% |\k@cgs@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in cgs units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@MassElectron}{% +\DeclareRobustCommand{\k@cgs@short@Rydberg}{% \ensuremath{% -9.108\expandafter\physconst@decimalsseparator% -980\expandafter\physconst@decimalsseparator% -087\expandafter\physconst@decimalsseparator% -382% -\times 10^{-31}\gm}} +2.18% +\times 10^{-11}\erg}} % \end{macrocode} % \end{macro} % @@ -2608,16 +9164,37 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@MassElectron} -% |\k@eV@short@MassElectron| is the mass of an electron in eV with reduced -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@full@Rydberg} +% |\k@cgs@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in cgs units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@MassElectron}{% +\DeclareRobustCommand{\k@cgs@full@Rydberg}{% +\ensuremath{% +2.179\expandafter\physconst@decimalsseparator% +775\expandafter\physconst@decimalsseparator% +77% +\times 10^{-11}\erg}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@Rydberg} +% |\k@eV@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in eV with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@eV@short@Rydberg}{% \ensuremath{% -5.69% -\times 10^{-19}\eV\,c^{-2}}} +1.36% +\times 10^{1}\eV}} % \end{macrocode} % \end{macro} % @@ -2627,19 +9204,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@MassElectron} -% |\k@eV@full@MassElectron| is the mass of an electron in eV with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@eV@full@Rydberg} +% |\k@eV@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% in eV with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@MassElectron}{% +\DeclareRobustCommand{\k@eV@full@Rydberg}{% \ensuremath{% -5.685\expandafter\physconst@decimalsseparator% -378\expandafter\physconst@decimalsseparator% -187\expandafter\physconst@decimalsseparator% -448% -\times 10^{-19}\eV\,c^{-2}}} +1.360\expandafter\physconst@decimalsseparator% +509\expandafter\physconst@decimalsseparator% +03% +\times 10^{1}\eV}} % \end{macrocode} % \end{macro} % @@ -2649,25 +9225,25 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kMassElectron} -% |\kMassElectron| is the mass of an electron. +% \begin{macro}{\kRydberg} +% |\kRydberg| is the Rydberg energy (the binding energy of Hydrogen). % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kMassElectron}{% -\k@SI@short@MassElectron} +\DeclareRobustCommand {\kRydberg}{% +\k@SI@short@Rydberg} \else -\DeclareRobustCommand {\kMassElectron}{% -\k@SI@full@MassElectron} +\DeclareRobustCommand {\kRydberg}{% +\k@SI@full@Rydberg} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kMassElectron}{% -\k@cgs@short@MassElectron} +\DeclareRobustCommand {\kRydberg}{% +\k@cgs@short@Rydberg} \else -\DeclareRobustCommand {\kMassElectron}{% -\k@cgs@full@MassElectron} +\DeclareRobustCommand {\kRydberg}{% +\k@cgs@full@Rydberg} \fi \fi % \end{macrocode} @@ -2679,17 +9255,107 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\keVMassElectron} -% |\keVMassElectron| is the mass of an electron. +% \begin{macro}{\keVRydberg} +% |\keVRydberg| is the Rydberg energy (the binding energy of Hydrogen). +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVRydberg}{% +\k@eV@short@Rydberg} +\else +\DeclareRobustCommand {\keVRydberg}{% +\k@eV@full@Rydberg} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@RydbergNumeric} +% |\k@SI@short@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen) +% in SI units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@RydbergNumeric}{% +\ensuremath{% +2.18e-18}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@RydbergNumeric} +% |\k@SI@full@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen) +% in SI units with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@RydbergNumeric}{% +\ensuremath{% +2.17977577e-18}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@RydbergNumeric} +% |\k@cgs@short@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen) +% in cgs units with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@RydbergNumeric}{% +\ensuremath{% +2.18e-11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@RydbergNumeric} +% |\k@cgs@full@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen) +% in cgs units with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@RydbergNumeric}{% +\ensuremath{% +2.17977577e-11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@eV@short@RydbergNumeric} +% |\k@eV@short@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen) +% in eV with reduced precision. +% Source: Calculated % % \begin{macrocode} -\ifx\shortconst\undefined -\DeclareRobustCommand {\keVMassElectron}{% -\k@eV@short@MassElectron} -\else -\DeclareRobustCommand {\keVMassElectron}{% -\k@eV@full@MassElectron} -\fi +\DeclareRobustCommand{\k@eV@short@RydbergNumeric}{% +\ensuremath{% +1.36e+01}} % \end{macrocode} % \end{macro} % @@ -2699,16 +9365,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@MassProton} -% |\k@SI@short@MassProton| is the mass of a proton in SI units with reduced -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@eV@full@RydbergNumeric} +% |\k@eV@full@RydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen) +% in eV with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@MassProton}{% +\DeclareRobustCommand{\k@eV@full@RydbergNumeric}{% \ensuremath{% -1.67% -\times 10^{-30}\kg}} +1.36050903e+01}} % \end{macrocode} % \end{macro} % @@ -2718,19 +9383,27 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@MassProton} -% |\k@SI@full@MassProton| is the mass of a proton in SI units with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\kRydbergNumeric} +% |\kRydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen). % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@MassProton}{% -\ensuremath{% -1.672\expandafter\physconst@decimalsseparator% -547\expandafter\physconst@decimalsseparator% -813\expandafter\physconst@decimalsseparator% -969% -\times 10^{-30}\kg}} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRydbergNumeric}{% +\k@SI@short@RydbergNumeric} +\else +\DeclareRobustCommand {\kRydbergNumeric}{% +\k@SI@full@RydbergNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRydbergNumeric}{% +\k@cgs@short@RydbergNumeric} +\else +\DeclareRobustCommand {\kRydbergNumeric}{% +\k@cgs@full@RydbergNumeric} +\fi +\fi % \end{macrocode} % \end{macro} % @@ -2740,16 +9413,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@MassProton} -% |\k@cgs@short@MassProton| is the mass of a proton in cgs units with reduced -% precision. -% Source: CODATA~2018 +% \begin{macro}{\keVRydbergNumeric} +% |\keVRydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen). % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@MassProton}{% -\ensuremath{% -1.67% -\times 10^{-27}\gm}} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVRydbergNumeric}{% +\k@eV@short@RydbergNumeric} +\else +\DeclareRobustCommand {\keVRydbergNumeric}{% +\k@eV@full@RydbergNumeric} +\fi % \end{macrocode} % \end{macro} % @@ -2759,19 +9433,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@MassProton} -% |\k@cgs@full@MassProton| is the mass of a proton in cgs units with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@short@LuminositySun} +% |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@MassProton}{% +\DeclareRobustCommand{\k@SI@short@LuminositySun}{% \ensuremath{% -1.672\expandafter\physconst@decimalsseparator% -547\expandafter\physconst@decimalsseparator% -813\expandafter\physconst@decimalsseparator% -969% -\times 10^{-27}\gm}} +3.83% +\times 10^{26}\Watt}} % \end{macrocode} % \end{macro} % @@ -2781,15 +9452,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@MassProton} -% |\k@eV@short@MassProton| is the mass of a proton in eV with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@LuminositySun} +% |\k@SI@full@LuminositySun| is the luminosity of the Sun in SI units with full +% precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@MassProton}{% +\DeclareRobustCommand{\k@SI@full@LuminositySun}{% \ensuremath{% -1.04% -\times 10^{-15}\eV\,c^{-2}}} +3.828% +\times 10^{26}\Watt}} % \end{macrocode} % \end{macro} % @@ -2799,18 +9471,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@MassProton} -% |\k@eV@full@MassProton| is the mass of a proton in eV with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@LuminositySun} +% |\k@cgs@short@LuminositySun| is the luminosity of the Sun in cgs units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@MassProton}{% +\DeclareRobustCommand{\k@cgs@short@LuminositySun}{% \ensuremath{% -1.043\expandafter\physconst@decimalsseparator% -922\expandafter\physconst@decimalsseparator% -235\expandafter\physconst@decimalsseparator% -836% -\times 10^{-15}\eV\,c^{-2}}} +3.83% +\times 10^{33}\erg\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -2820,27 +9490,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kMassProton} -% |\kMassProton| is the mass of a proton. +% \begin{macro}{\k@cgs@full@LuminositySun} +% |\k@cgs@full@LuminositySun| is the luminosity of the Sun in cgs units with +% full precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kMassProton}{% -\k@SI@short@MassProton} -\else -\DeclareRobustCommand {\kMassProton}{% -\k@SI@full@MassProton} -\fi -\else -\ifx\shortconst\undefined -\DeclareRobustCommand {\kMassProton}{% -\k@cgs@short@MassProton} -\else -\DeclareRobustCommand {\kMassProton}{% -\k@cgs@full@MassProton} -\fi -\fi +\DeclareRobustCommand{\k@cgs@full@LuminositySun}{% +\ensuremath{% +3.828% +\times 10^{33}\erg\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -2850,16 +9509,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\keVMassProton} -% |\keVMassProton| is the mass of a proton. +% \begin{macro}{\kLuminositySun} +% |\kLuminositySun| is the luminosity of the Sun. % % \begin{macrocode} +\ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\keVMassProton}{% -\k@eV@short@MassProton} +\DeclareRobustCommand {\kLuminositySun}{% +\k@SI@short@LuminositySun} \else -\DeclareRobustCommand {\keVMassProton}{% -\k@eV@full@MassProton} +\DeclareRobustCommand {\kLuminositySun}{% +\k@SI@full@LuminositySun} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kLuminositySun}{% +\k@cgs@short@LuminositySun} +\else +\DeclareRobustCommand {\kLuminositySun}{% +\k@cgs@full@LuminositySun} +\fi \fi % \end{macrocode} % \end{macro} @@ -2870,16 +9539,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@MassHydrogen} -% |\k@SI@short@MassHydrogen| is the mass of a neutral hydrogen atom in SI units -% with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@short@LuminositySunNumeric} +% |\k@SI@short@LuminositySunNumeric| is the luminosity of the Sun in SI units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@MassHydrogen}{% +\DeclareRobustCommand{\k@SI@short@LuminositySunNumeric}{% \ensuremath{% -1.67% -\times 10^{-30}\kg}} +3.83e+26}} % \end{macrocode} % \end{macro} % @@ -2889,19 +9557,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@MassHydrogen} -% |\k@SI@full@MassHydrogen| is the mass of a neutral hydrogen atom in SI units -% with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@LuminositySunNumeric} +% |\k@SI@full@LuminositySunNumeric| is the luminosity of the Sun in SI units with full +% precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@MassHydrogen}{% +\DeclareRobustCommand{\k@SI@full@LuminositySunNumeric}{% \ensuremath{% -1.673\expandafter\physconst@decimalsseparator% -458\expandafter\physconst@decimalsseparator% -687\expandafter\physconst@decimalsseparator% -724% -\times 10^{-30}\kg}} +3.828e+26}} % \end{macrocode} % \end{macro} % @@ -2911,16 +9575,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@MassHydrogen} -% |\k@cgs@short@MassHydrogen| is the mass of a neutral hydrogen atom in cgs -% units with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@LuminositySunNumeric} +% |\k@cgs@short@LuminositySunNumeric| is the luminosity of the Sun in cgs units with +% reduced precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@MassHydrogen}{% +\DeclareRobustCommand{\k@cgs@short@LuminositySunNumeric}{% \ensuremath{% -1.67% -\times 10^{-27}\gm}} +3.83e+33}} % \end{macrocode} % \end{macro} % @@ -2930,19 +9593,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@MassHydrogen} -% |\k@cgs@full@MassHydrogen| is the mass of a neutral hydrogen atom in cgs -% units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@full@LuminositySunNumeric} +% |\k@cgs@full@LuminositySunNumeric| is the luminosity of the Sun in cgs units with +% full precision. +% Source: IAU~Resolution~B3~2015 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@MassHydrogen}{% +\DeclareRobustCommand{\k@cgs@full@LuminositySunNumeric}{% \ensuremath{% -1.673\expandafter\physconst@decimalsseparator% -458\expandafter\physconst@decimalsseparator% -687\expandafter\physconst@decimalsseparator% -724% -\times 10^{-27}\gm}} +3.828e+33}} % \end{macrocode} % \end{macro} % @@ -2952,38 +9611,50 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@MassHydrogen} -% |\k@eV@short@MassHydrogen| is the mass of a neutral hydrogen atom in eV with -% reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\kLuminositySunNumeric} +% |\kLuminositySunNumeric| is the luminosity of the Sun. % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@MassHydrogen}{% -\ensuremath{% -1.04% -\times 10^{-15}\eV\,c^{-2}}} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kLuminositySunNumeric}{% +\k@SI@short@LuminositySunNumeric} +\else +\DeclareRobustCommand {\kLuminositySunNumeric}{% +\k@SI@full@LuminositySunNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kLuminositySunNumeric}{% +\k@cgs@short@LuminositySunNumeric} +\else +\DeclareRobustCommand {\kLuminositySunNumeric}{% +\k@cgs@full@LuminositySunNumeric} +\fi +\fi % \end{macrocode} % \end{macro} % %\iffalse % %\fi +% +%\subsection{Pressure} +% %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@MassHydrogen} -% |\k@eV@full@MassHydrogen| is the mass of a neutral hydrogen atom in eV with -% full precision. +% \begin{macro}{\k@SI@short@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureAtmosphere| is the standard atmospheric pressure in SI +% units with reduced precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@MassHydrogen}{% +\DeclareRobustCommand{\k@SI@short@PressureAtmosphere}{% \ensuremath{% -1.044\expandafter\physconst@decimalsseparator% -490\expandafter\physconst@decimalsseparator% -758\expandafter\physconst@decimalsseparator% -517% -\times 10^{-15}\eV\,c^{-2}}} +1.01% +\times 10^{5}\Pa}} % \end{macrocode} % \end{macro} % @@ -2993,27 +9664,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kMassHydrogen} -% |\kMassHydrogen| is the mass of a neutral hydrogen atom. +% \begin{macro}{\k@SI@full@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureAtmosphere| is the standard atmospheric pressure in SI +% units with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kMassHydrogen}{% -\k@SI@short@MassHydrogen} -\else -\DeclareRobustCommand {\kMassHydrogen}{% -\k@SI@full@MassHydrogen} -\fi -\else -\ifx\shortconst\undefined -\DeclareRobustCommand {\kMassHydrogen}{% -\k@cgs@short@MassHydrogen} -\else -\DeclareRobustCommand {\kMassHydrogen}{% -\k@cgs@full@MassHydrogen} -\fi -\fi +\DeclareRobustCommand{\k@SI@full@PressureAtmosphere}{% +\ensuremath{% +1.013\expandafter\physconst@decimalsseparator% +25% +\times 10^{5}\Pa}} % \end{macrocode} % \end{macro} % @@ -3023,17 +9685,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\keVMassHydrogen} -% |\keVMassHydrogen| is the mass of a neutral hydrogen atom. +% \begin{macro}{\k@cgs@short@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureAtmosphere| is the standard atmospheric pressure in cgs +% units with reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\ifx\shortconst\undefined -\DeclareRobustCommand {\keVMassHydrogen}{% -\k@eV@short@MassHydrogen} -\else -\DeclareRobustCommand {\keVMassHydrogen}{% -\k@eV@full@MassHydrogen} -\fi +\DeclareRobustCommand{\k@cgs@short@PressureAtmosphere}{% +\ensuremath{% +1.01\barP}} % \end{macrocode} % \end{macro} % @@ -3043,16 +9704,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@MassSun} -% |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced -% precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@cgs@full@PressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureAtmosphere| is the standard atmospheric pressure in cgs +% units with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@MassSun}{% +\DeclareRobustCommand{\k@cgs@full@PressureAtmosphere}{% \ensuremath{% -1.99% -\times 10^{30}\kg}} +1.013\expandafter\physconst@decimalsseparator% +25\barP}} % \end{macrocode} % \end{macro} % @@ -3062,17 +9724,28 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@MassSun} -% |\k@SI@full@MassSun| is the mass of the Sun in SI units with full precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\kPressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\kPressureAtmosphere| is the standard atmospheric pressure. % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@MassSun}{% -\ensuremath{% -1.988\expandafter\physconst@decimalsseparator% -409\expandafter\physconst@decimalsseparator% -9% -\times 10^{30}\kg}} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPressureAtmosphere}{% +\k@SI@short@PressureAtmosphere} +\else +\DeclareRobustCommand {\kPressureAtmosphere}{% +\k@SI@full@PressureAtmosphere} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPressureAtmosphere}{% +\k@cgs@short@PressureAtmosphere} +\else +\DeclareRobustCommand {\kPressureAtmosphere}{% +\k@cgs@full@PressureAtmosphere} +\fi +\fi % \end{macrocode} % \end{macro} % @@ -3082,16 +9755,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@MassSun} -% |\k@cgs@short@MassSun| is the mass of the Sun in cgs units with reduced -% precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@SI@short@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureAtmosphereNumeric| is the standard atmospheric pressure in SI +% units with reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@MassSun}{% +\DeclareRobustCommand{\k@SI@short@PressureAtmosphereNumeric}{% \ensuremath{% -1.99% -\times 10^{33}\gm}} +1.01e+05}} % \end{macrocode} % \end{macro} % @@ -3101,17 +9774,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@MassSun} -% |\k@cgs@full@MassSun| is the mass of the Sun in cgs units with full precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@SI@full@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureAtmosphereNumeric| is the standard atmospheric pressure in SI +% units with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@MassSun}{% +\DeclareRobustCommand{\k@SI@full@PressureAtmosphereNumeric}{% \ensuremath{% -1.988\expandafter\physconst@decimalsseparator% -409\expandafter\physconst@decimalsseparator% -9% -\times 10^{33}\gm}} +1.01325e+05}} % \end{macrocode} % \end{macro} % @@ -3121,27 +9793,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kMassSun} -% |\kMassSun| is the mass of the Sun. +% \begin{macro}{\k@cgs@short@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureAtmosphereNumeric| is the standard atmospheric pressure in cgs +% units with reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kMassSun}{% -\k@SI@short@MassSun} -\else -\DeclareRobustCommand {\kMassSun}{% -\k@SI@full@MassSun} -\fi -\else -\ifx\shortconst\undefined -\DeclareRobustCommand {\kMassSun}{% -\k@cgs@short@MassSun} -\else -\DeclareRobustCommand {\kMassSun}{% -\k@cgs@full@MassSun} -\fi -\fi +\DeclareRobustCommand{\k@cgs@short@PressureAtmosphereNumeric}{% +\ensuremath{% +1.01e+00}} % \end{macrocode} % \end{macro} % @@ -3151,16 +9812,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@MassAMU} -% |\k@SI@short@MassAMU| is the mass of an atomic mass unit in SI units with -% reduced precision. +% \begin{macro}{\k@cgs@full@PressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureAtmosphereNumeric| is the standard atmospheric pressure in cgs +% units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@MassAMU}{% +\DeclareRobustCommand{\k@cgs@full@PressureAtmosphereNumeric}{% \ensuremath{% -1.66% -\times 10^{-30}\kg}} +1.01325e+00}} % \end{macrocode} % \end{macro} % @@ -3170,19 +9831,28 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@MassAMU} -% |\k@SI@full@MassAMU| is the mass of an atomic mass unit in SI units with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\kPressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\kPressureAtmosphereNumeric| is the standard atmospheric pressure. % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@MassAMU}{% -\ensuremath{% -1.660\expandafter\physconst@decimalsseparator% -465\expandafter\physconst@decimalsseparator% -492\expandafter\physconst@decimalsseparator% -239% -\times 10^{-30}\kg}} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPressureAtmosphereNumeric}{% +\k@SI@short@PressureAtmosphereNumeric} +\else +\DeclareRobustCommand {\kPressureAtmosphereNumeric}{% +\k@SI@full@PressureAtmosphereNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPressureAtmosphereNumeric}{% +\k@cgs@short@PressureAtmosphereNumeric} +\else +\DeclareRobustCommand {\kPressureAtmosphereNumeric}{% +\k@cgs@full@PressureAtmosphereNumeric} +\fi +\fi % \end{macrocode} % \end{macro} % @@ -3192,16 +9862,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@MassAMU} -% |\k@cgs@short@MassAMU| is the mass of an atomic mass unit in cgs units with -% reduced precision. +% \begin{macro}{\k@SI@short@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureStandard| is the standard atmospheric pressure in SI +% units with reduced precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@MassAMU}{% +\DeclareRobustCommand{\k@SI@short@PressureStandard}{% \ensuremath{% -1.66% -\times 10^{-27}\gm}} +1.00% +\times 10^{5}\Pa}} % \end{macrocode} % \end{macro} % @@ -3211,19 +9882,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@MassAMU} -% |\k@cgs@full@MassAMU| is the mass of an atomic mass unit in cgs units with -% full precision. +% \begin{macro}{\k@SI@full@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureStandard| is the standard atmospheric pressure in SI +% units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@MassAMU}{% +\DeclareRobustCommand{\k@SI@full@PressureStandard}{% \ensuremath{% -1.660\expandafter\physconst@decimalsseparator% -465\expandafter\physconst@decimalsseparator% -492\expandafter\physconst@decimalsseparator% -239% -\times 10^{-27}\gm}} +1.000\expandafter\physconst@decimalsseparator% +00% +\times 10^{5}\Pa}} % \end{macrocode} % \end{macro} % @@ -3233,16 +9903,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@MassAMU} -% |\k@eV@short@MassAMU| is the mass of an atomic mass unit in eV with reduced -% precision. +% \begin{macro}{\k@cgs@short@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureStandard| is the standard atmospheric pressure in cgs +% units with reduced precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@MassAMU}{% +\DeclareRobustCommand{\k@cgs@short@PressureStandard}{% \ensuremath{% -1.04% -\times 10^{-15}\eV\,c^{-2}}} +1.00\barP}} % \end{macrocode} % \end{macro} % @@ -3252,19 +9922,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@MassAMU} -% |\k@eV@full@MassAMU| is the mass of an atomic mass unit in eV with full -% precision. +% \begin{macro}{\k@cgs@full@PressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureStandard| is the standard atmospheric pressure in cgs +% units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@MassAMU}{% +\DeclareRobustCommand{\k@cgs@full@PressureStandard}{% \ensuremath{% -1.036\expandafter\physconst@decimalsseparator% -381\expandafter\physconst@decimalsseparator% -043\expandafter\physconst@decimalsseparator% -764% -\times 10^{-15}\eV\,c^{-2}}} +1.000\expandafter\physconst@decimalsseparator% +00\barP}} % \end{macrocode} % \end{macro} % @@ -3274,46 +9942,27 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kMassAMU} -% |\kMassAMU| is the mass of an atomic mass unit. +% \begin{macro}{\kPressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\kPressureStandard| is the standard atmospheric pressure. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kMassAMU}{% -\k@SI@short@MassAMU} +\DeclareRobustCommand {\kPressureStandard}{% +\k@SI@short@PressureStandard} \else -\DeclareRobustCommand {\kMassAMU}{% -\k@SI@full@MassAMU} +\DeclareRobustCommand {\kPressureStandard}{% +\k@SI@full@PressureStandard} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kMassAMU}{% -\k@cgs@short@MassAMU} +\DeclareRobustCommand {\kPressureStandard}{% +\k@cgs@short@PressureStandard} \else -\DeclareRobustCommand {\kMassAMU}{% -\k@cgs@full@MassAMU} -\fi +\DeclareRobustCommand {\kPressureStandard}{% +\k@cgs@full@PressureStandard} \fi -% \end{macrocode} -% \end{macro} -% -%\iffalse -% -%\fi -%\iffalse -%<*package> -%\fi -% \begin{macro}{\keVMassAMU} -% |\keVMassAMU| is the mass of an atomic mass unit. -% -% \begin{macrocode} -\ifx\shortconst\undefined -\DeclareRobustCommand {\keVMassAMU}{% -\k@eV@short@MassAMU} -\else -\DeclareRobustCommand {\keVMassAMU}{% -\k@eV@full@MassAMU} \fi % \end{macrocode} % \end{macro} @@ -3321,22 +9970,19 @@ %\iffalse % %\fi -% -%\subsection{Charge} -% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@ChargeFundamental} -% |\k@SI@short@ChargeFundamental| is the fundamental charge in SI units with -% reduced precision. +% \begin{macro}{\k@SI@short@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@short@PressureStandardNumeric| is the standard atmospheric pressure in SI +% units with reduced precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@ChargeFundamental}{% +\DeclareRobustCommand{\k@SI@short@PressureStandardNumeric}{% \ensuremath{% -1.60% -\times 10^{-19}\Coulomb}} +1.00e+05}} % \end{macrocode} % \end{macro} % @@ -3346,18 +9992,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@ChargeFundamental} -% |\k@SI@full@ChargeFundamental| is the fundamental charge in SI units with -% full precision. +% \begin{macro}{\k@SI@full@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@SI@full@PressureStandardNumeric| is the standard atmospheric pressure in SI +% units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@ChargeFundamental}{% +\DeclareRobustCommand{\k@SI@full@PressureStandardNumeric}{% \ensuremath{% -1.602\expandafter\physconst@decimalsseparator% -176\expandafter\physconst@decimalsseparator% -634% -\times 10^{-19}\Coulomb}} +1.00000e+05}} % \end{macrocode} % \end{macro} % @@ -3367,16 +10011,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@ChargeFundamental} -% |\k@cgs@short@ChargeFundamental| is the fundamental charge in cgs units with -% reduced precision. +% \begin{macro}{\k@cgs@short@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@short@PressureStandardNumeric| is the standard atmospheric pressure in cgs +% units with reduced precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@ChargeFundamental}{% +\DeclareRobustCommand{\k@cgs@short@PressureStandardNumeric}{% \ensuremath{% -4.80% -\times 10^{-10}\esu}} +1.00e+00}} % \end{macrocode} % \end{macro} % @@ -3386,18 +10030,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@ChargeFundamental} -% |\k@cgs@full@ChargeFundamental| is the fundamental charge in cgs units with -% full precision. +% \begin{macro}{\k@cgs@full@PressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\k@cgs@full@PressureStandardNumeric| is the standard atmospheric pressure in cgs +% units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@ChargeFundamental}{% +\DeclareRobustCommand{\k@cgs@full@PressureStandardNumeric}{% \ensuremath{% -4.803\expandafter\physconst@decimalsseparator% -204\expandafter\physconst@decimalsseparator% -713% -\times 10^{-10}\esu}} +1.00000e+00}} % \end{macrocode} % \end{macro} % @@ -3407,25 +10049,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kChargeFundamental} -% |\kChargeFundamental| is the fundamental charge. +% \begin{macro}{\kPressureStandardNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\kPressureStandardNumeric| is the standard atmospheric pressure. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kChargeFundamental}{% -\k@SI@short@ChargeFundamental} +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@SI@short@PressureStandardNumeric} \else -\DeclareRobustCommand {\kChargeFundamental}{% -\k@SI@full@ChargeFundamental} +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@SI@full@PressureStandardNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kChargeFundamental}{% -\k@cgs@short@ChargeFundamental} +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@cgs@short@PressureStandardNumeric} \else -\DeclareRobustCommand {\kChargeFundamental}{% -\k@cgs@full@ChargeFundamental} +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@cgs@full@PressureStandardNumeric} \fi \fi % \end{macrocode} @@ -3434,19 +10077,22 @@ %\iffalse % %\fi +% +%\subsection{Velocity, Speed and Acceleration} +% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@ChargeElectron} -% |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with -% reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@short@SpeedLight} +% |\k@SI@short@SpeedLight| is the speed of light in SI units with reduced +% precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@ChargeElectron}{% +\DeclareRobustCommand{\k@SI@short@SpeedLight}{% \ensuremath{% --1.60% -\times 10^{-19}\Coulomb}} +3.00% +\times 10^{8}\m\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -3456,18 +10102,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@ChargeElectron} -% |\k@SI@full@ChargeElectron| is the charge of an electron in SI units with -% full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@SpeedLight} +% |\k@SI@full@SpeedLight| is the speed of light in SI units with full precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@ChargeElectron}{% +\DeclareRobustCommand{\k@SI@full@SpeedLight}{% \ensuremath{% --1.602\expandafter\physconst@decimalsseparator% -176\expandafter\physconst@decimalsseparator% -634% -\times 10^{-19}\Coulomb}} +2.997\expandafter\physconst@decimalsseparator% +924\expandafter\physconst@decimalsseparator% +58% +\times 10^{8}\m\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -3477,16 +10122,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@ChargeElectron} -% |\k@cgs@short@ChargeElectron| is the charge of an electron in cgs units with -% reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@SpeedLight} +% |\k@cgs@short@SpeedLight| is the speed of light in cgs units with reduced +% precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@ChargeElectron}{% +\DeclareRobustCommand{\k@cgs@short@SpeedLight}{% \ensuremath{% --4.80% -\times 10^{-10}\esu}} +3.00% +\times 10^{10}\cm\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -3496,18 +10141,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@ChargeElectron} -% |\k@cgs@full@ChargeElectron| is the charge of an electron in cgs units with -% full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@full@SpeedLight} +% |\k@cgs@full@SpeedLight| is the speed of light in cgs units with full +% precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@ChargeElectron}{% +\DeclareRobustCommand{\k@cgs@full@SpeedLight}{% \ensuremath{% --4.803\expandafter\physconst@decimalsseparator% -204\expandafter\physconst@decimalsseparator% -713% -\times 10^{-10}\esu}} +2.997\expandafter\physconst@decimalsseparator% +924\expandafter\physconst@decimalsseparator% +58% +\times 10^{10}\cm\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -3517,25 +10162,25 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kChargeElectron} -% |\kChargeElectron| is the charge of an electron. +% \begin{macro}{\kSpeedLight} +% |\kSpeedLight| is the speed of light. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kChargeElectron}{% -\k@SI@short@ChargeElectron} +\DeclareRobustCommand {\kSpeedLight}{% +\k@SI@short@SpeedLight} \else -\DeclareRobustCommand {\kChargeElectron}{% -\k@SI@full@ChargeElectron} +\DeclareRobustCommand {\kSpeedLight}{% +\k@SI@full@SpeedLight} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kChargeElectron}{% -\k@cgs@short@ChargeElectron} +\DeclareRobustCommand {\kSpeedLight}{% +\k@cgs@short@SpeedLight} \else -\DeclareRobustCommand {\kChargeElectron}{% -\k@cgs@full@ChargeElectron} +\DeclareRobustCommand {\kSpeedLight}{% +\k@cgs@full@SpeedLight} \fi \fi % \end{macrocode} @@ -3547,16 +10192,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@ChargeProton} -% |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced +% \begin{macro}{\k@SI@short@SpeedLightNumeric} +% |\k@SI@short@SpeedLightNumeric| is the speed of light in SI units with reduced % precision. -% Source: CODATA~2018 +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@ChargeProton}{% +\DeclareRobustCommand{\k@SI@short@SpeedLightNumeric}{% \ensuremath{% -1.60% -\times 10^{-19}\Coulomb}} +3.00e+08}} % \end{macrocode} % \end{macro} % @@ -3566,18 +10210,14 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@ChargeProton} -% |\k@SI@full@ChargeProton| is the charge of a proton in SI units with full -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@SpeedLightNumeric} +% |\k@SI@full@SpeedLightNumeric| is the speed of light in SI units with full precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@ChargeProton}{% +\DeclareRobustCommand{\k@SI@full@SpeedLightNumeric}{% \ensuremath{% -1.602\expandafter\physconst@decimalsseparator% -176\expandafter\physconst@decimalsseparator% -634% -\times 10^{-19}\Coulomb}} +2.99792458e+08}} % \end{macrocode} % \end{macro} % @@ -3587,16 +10227,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@ChargeProton} -% |\k@cgs@short@ChargeProton| is the charge of a proton in cgs units with -% reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@SpeedLightNumeric} +% |\k@cgs@short@SpeedLightNumeric| is the speed of light in cgs units with reduced +% precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@ChargeProton}{% +\DeclareRobustCommand{\k@cgs@short@SpeedLightNumeric}{% \ensuremath{% -4.80% -\times 10^{-10}\esu}} +3.00e+10}} % \end{macrocode} % \end{macro} % @@ -3606,18 +10245,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@ChargeProton} -% |\k@cgs@full@ChargeProton| is the charge of a proton in cgs units with full +% \begin{macro}{\k@cgs@full@SpeedLightNumeric} +% |\k@cgs@full@SpeedLightNumeric| is the speed of light in cgs units with full % precision. -% Source: CODATA~2018 +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@ChargeProton}{% +\DeclareRobustCommand{\k@cgs@full@SpeedLightNumeric}{% \ensuremath{% -4.803\expandafter\physconst@decimalsseparator% -204\expandafter\physconst@decimalsseparator% -713% -\times 10^{-10}\esu}} +2.99792458e+10}} % \end{macrocode} % \end{macro} % @@ -3627,25 +10263,25 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kChargeProton} -% |\kChargeProton| is the charge of a proton. +% \begin{macro}{\kSpeedLightNumeric} +% |\kSpeedLightNumeric| is the speed of light. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kChargeProton}{% -\k@SI@short@ChargeProton} +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@SI@short@SpeedLightNumeric} \else -\DeclareRobustCommand {\kChargeProton}{% -\k@SI@full@ChargeProton} +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@SI@full@SpeedLightNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kChargeProton}{% -\k@cgs@short@ChargeProton} +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@cgs@short@SpeedLightNumeric} \else -\DeclareRobustCommand {\kChargeProton}{% -\k@cgs@full@ChargeProton} +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@cgs@full@SpeedLightNumeric} \fi \fi % \end{macrocode} @@ -3654,22 +10290,20 @@ %\iffalse % %\fi -% -%\subsection{Distances and Lengths} -% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@RadiusBohr} -% |\k@SI@short@RadiusBohr| is Bohr radius of an atom in SI units with reduced -% precision. -% Source: Calculated +% \begin{macro}{\k@SI@short@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@short@AccelGravity| is the accelertion due to gravity at the surface +% of the Earth in SI units with reduced precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@RadiusBohr}{% +\DeclareRobustCommand{\k@SI@short@AccelGravity}{% \ensuremath{% -5.29% -\times 10^{-8}\m}} +9.81\m\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -3679,18 +10313,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@RadiusBohr} -% |\k@SI@full@RadiusBohr| is Bohr radius of an atom in SI units with full -% precision. -% Source: Calculated +% \begin{macro}{\k@SI@full@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@full@AccelGravity| is the accelertion due to gravity at the surface of +% the Earth in SI units with full precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@RadiusBohr}{% +\DeclareRobustCommand{\k@SI@full@AccelGravity}{% \ensuremath{% -5.292\expandafter\physconst@decimalsseparator% -006\expandafter\physconst@decimalsseparator% -59% -\times 10^{-8}\m}} +9.806\expandafter\physconst@decimalsseparator% +65\m\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -3700,16 +10334,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@RadiusBohr} -% |\k@cgs@short@RadiusBohr| is Bohr radius of an atom in cgs units with reduced -% precision. -% Source: Calculated +% \begin{macro}{\k@cgs@short@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@short@AccelGravity| is the accelertion due to gravity at the surface +% of the Earth in cgs units with reduced precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@RadiusBohr}{% +\DeclareRobustCommand{\k@cgs@short@AccelGravity}{% \ensuremath{% -5.29% -\times 10^{-6}\cm}} +9.81% +\times 10^{2}\cm\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -3719,18 +10355,19 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@RadiusBohr} -% |\k@cgs@full@RadiusBohr| is Bohr radius of an atom in cgs units with full -% precision. -% Source: Calculated +% \begin{macro}{\k@cgs@full@AccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@full@AccelGravity| is the accelertion due to gravity at the surface +% of the Earth in cgs units with full precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@RadiusBohr}{% +\DeclareRobustCommand{\k@cgs@full@AccelGravity}{% \ensuremath{% -5.292\expandafter\physconst@decimalsseparator% -006\expandafter\physconst@decimalsseparator% -59% -\times 10^{-6}\cm}} +9.806\expandafter\physconst@decimalsseparator% +65% +\times 10^{2}\cm\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -3740,25 +10377,28 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kRadiusBohr} -% |\kRadiusBohr| is Bohr radius of an atom. +% \begin{macro}{\kAccelGravity} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\kAccelGravity| is the accelertion due to gravity at the surface of the +% Earth. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kRadiusBohr}{% -\k@SI@short@RadiusBohr} +\DeclareRobustCommand {\kAccelGravity}{% +\k@SI@short@AccelGravity} \else -\DeclareRobustCommand {\kRadiusBohr}{% -\k@SI@full@RadiusBohr} +\DeclareRobustCommand {\kAccelGravity}{% +\k@SI@full@AccelGravity} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kRadiusBohr}{% -\k@cgs@short@RadiusBohr} +\DeclareRobustCommand {\kAccelGravity}{% +\k@cgs@short@AccelGravity} \else -\DeclareRobustCommand {\kRadiusBohr}{% -\k@cgs@full@RadiusBohr} +\DeclareRobustCommand {\kAccelGravity}{% +\k@cgs@full@AccelGravity} \fi \fi % \end{macrocode} @@ -3770,16 +10410,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@AstronomicalUnit} -% |\k@SI@short@AstronomicalUnit| is the astronomical unit (the average distance -% between the Earth and the Sun) in SI units with reduced precision. -% Source: IAU~Resolution~B2~2012 +% \begin{macro}{\k@SI@short@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@short@AccelGravityNumeric| is the accelertion due to gravity at the surface +% of the Earth in SI units with reduced precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@AstronomicalUnit}{% +\DeclareRobustCommand{\k@SI@short@AccelGravityNumeric}{% \ensuremath{% -1.50% -\times 10^{11}\m}} +9.81e+00}} % \end{macrocode} % \end{macro} % @@ -3789,18 +10430,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@AstronomicalUnit} -% |\k@SI@full@AstronomicalUnit| is the astronomical unit (the average distance -% between the Earth and the Sun) in SI units with full precision. -% Source: IAU~Resolution~B2~2012 +% \begin{macro}{\k@SI@full@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@SI@full@AccelGravityNumeric| is the accelertion due to gravity at the surface of +% the Earth in SI units with full precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@AstronomicalUnit}{% +\DeclareRobustCommand{\k@SI@full@AccelGravityNumeric}{% \ensuremath{% -1.495\expandafter\physconst@decimalsseparator% -978\expandafter\physconst@decimalsseparator% -707% -\times 10^{11}\m}} +9.80665e+00}} % \end{macrocode} % \end{macro} % @@ -3810,16 +10450,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@AstronomicalUnit} -% |\k@cgs@short@AstronomicalUnit| is the astronomical unit (the average -% distance between the Earth and the Sun) in cgs units with reduced precision. -% Source: IAU~Resolution~B2~2012 +% \begin{macro}{\k@cgs@short@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@short@AccelGravityNumeric| is the accelertion due to gravity at the surface +% of the Earth in cgs units with reduced precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@AstronomicalUnit}{% +\DeclareRobustCommand{\k@cgs@short@AccelGravityNumeric}{% \ensuremath{% -1.50% -\times 10^{13}\cm}} +9.81e+02}} % \end{macrocode} % \end{macro} % @@ -3829,18 +10470,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@AstronomicalUnit} -% |\k@cgs@full@AstronomicalUnit| is the astronomical unit (the average distance -% between the Earth and the Sun) in cgs units with full precision. -% Source: IAU~Resolution~B2~2012 +% \begin{macro}{\k@cgs@full@AccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\k@cgs@full@AccelGravityNumeric| is the accelertion due to gravity at the surface +% of the Earth in cgs units with full precision. +% Source: CODATA 2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@AstronomicalUnit}{% +\DeclareRobustCommand{\k@cgs@full@AccelGravityNumeric}{% \ensuremath{% -1.495\expandafter\physconst@decimalsseparator% -978\expandafter\physconst@decimalsseparator% -707% -\times 10^{13}\cm}} +9.80665e+02}} % \end{macrocode} % \end{macro} % @@ -3850,26 +10490,28 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kAstronomicalUnit} -% |\kAstronomicalUnit| is the astronomical unit (the average distance between -% the Earth and the Sun). +% \begin{macro}{\kAccelGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Correct value.} +% \changes{v1.1.0}{2020/02/03}{Fix units.} +% |\kAccelGravityNumeric| is the accelertion due to gravity at the surface of the +% Earth. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kAstronomicalUnit}{% -\k@SI@short@AstronomicalUnit} +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@SI@short@AccelGravityNumeric} \else -\DeclareRobustCommand {\kAstronomicalUnit}{% -\k@SI@full@AstronomicalUnit} +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@SI@full@AccelGravityNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kAstronomicalUnit}{% -\k@cgs@short@AstronomicalUnit} +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@cgs@short@AccelGravityNumeric} \else -\DeclareRobustCommand {\kAstronomicalUnit}{% -\k@cgs@full@AstronomicalUnit} +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@cgs@full@AccelGravityNumeric} \fi \fi % \end{macrocode} @@ -3878,19 +10520,23 @@ %\iffalse % %\fi +% +%\subsection{Other Constants} +% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@Parsec} -% |\k@SI@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% \begin{macro}{\k@SI@short@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in % SI units with reduced precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@Parsec}{% +\DeclareRobustCommand{\k@SI@short@Coulomb}{% \ensuremath{% -3.09% -\times 10^{16}\m}} +8.99% +\times 10^{9}\N\m^2\Coulomb^{-2}}} % \end{macrocode} % \end{macro} % @@ -3900,18 +10546,19 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@Parsec} -% |\k@SI@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in SI -% units with full precision. +% \begin{macro}{\k@SI@full@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% SI units with full precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@Parsec}{% +\DeclareRobustCommand{\k@SI@full@Coulomb}{% \ensuremath{% -3.085\expandafter\physconst@decimalsseparator% -677\expandafter\physconst@decimalsseparator% -581% -\times 10^{16}\m}} +8.987\expandafter\physconst@decimalsseparator% +551\expandafter\physconst@decimalsseparator% +79% +\times 10^{9}\N\m^2\Coulomb^{-2}}} % \end{macrocode} % \end{macro} % @@ -3920,17 +10567,17 @@ %\fi %\iffalse %<*package> -%\fi -% \begin{macro}{\k@cgs@short@Parsec} -% |\k@cgs@short@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in -% cgs units with reduced precision. +%\fi +% \begin{macro}{\k@cgs@short@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) +% in cgs units with reduced precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@Parsec}{% +\DeclareRobustCommand{\k@cgs@short@Coulomb}{% \ensuremath{% -3.09% -\times 10^{18}\cm}} +1.00}} % \end{macrocode} % \end{macro} % @@ -3940,18 +10587,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@Parsec} -% |\k@cgs@full@Parsec| is the length of a parsec ($\frac{648000\au}{\pi}$) in +% \begin{macro}{\k@cgs@full@Coulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in % cgs units with full precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@Parsec}{% +\DeclareRobustCommand{\k@cgs@full@Coulomb}{% \ensuremath{% -3.085\expandafter\physconst@decimalsseparator% -677\expandafter\physconst@decimalsseparator% -581% -\times 10^{18}\cm}} +1.000\expandafter\physconst@decimalsseparator% +000\expandafter\physconst@decimalsseparator% +00}} % \end{macrocode} % \end{macro} % @@ -3961,25 +10608,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kParsec} -% |\kParsec| is the length of a parsec ($\frac{648000\au}{\pi}$). +% \begin{macro}{\kCoulomb} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kCoulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$). % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kParsec}{% -\k@SI@short@Parsec} +\DeclareRobustCommand {\kCoulomb}{% +\k@SI@short@Coulomb} \else -\DeclareRobustCommand {\kParsec}{% -\k@SI@full@Parsec} +\DeclareRobustCommand {\kCoulomb}{% +\k@SI@full@Coulomb} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kParsec}{% -\k@cgs@short@Parsec} +\DeclareRobustCommand {\kCoulomb}{% +\k@cgs@short@Coulomb} \else -\DeclareRobustCommand {\kParsec}{% -\k@cgs@full@Parsec} +\DeclareRobustCommand {\kCoulomb}{% +\k@cgs@full@Coulomb} \fi \fi % \end{macrocode} @@ -3991,16 +10639,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@RadiusSun} -% |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with -% reduced precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@SI@short@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% SI units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@RadiusSun}{% +\DeclareRobustCommand{\k@SI@short@CoulombNumeric}{% \ensuremath{% -6.96% -\times 10^{8}\m}} +8.99e+09}} % \end{macrocode} % \end{macro} % @@ -4010,16 +10658,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@RadiusSun} -% |\k@SI@full@RadiusSun| is the mean radius of the Sun in SI units with full -% precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@SI@full@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% SI units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@RadiusSun}{% +\DeclareRobustCommand{\k@SI@full@CoulombNumeric}{% \ensuremath{% -6.957% -\times 10^{8}\m}} +8.98755179e+09}} % \end{macrocode} % \end{macro} % @@ -4029,16 +10677,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@RadiusSun} -% |\k@cgs@short@RadiusSun| is the mean radius of the Sun in cgs units with -% reduced precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@cgs@short@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) +% in cgs units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@RadiusSun}{% +\DeclareRobustCommand{\k@cgs@short@CoulombNumeric}{% \ensuremath{% -6.96% -\times 10^{10}\cm}} +1.00e+00}} % \end{macrocode} % \end{macro} % @@ -4048,16 +10696,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@RadiusSun} -% |\k@cgs@full@RadiusSun| is the mean radius of the Sun in cgs units with full -% precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@cgs@full@CoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@CoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in +% cgs units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@RadiusSun}{% +\DeclareRobustCommand{\k@cgs@full@CoulombNumeric}{% \ensuremath{% -6.957% -\times 10^{10}\cm}} +1.00000000e+00}} % \end{macrocode} % \end{macro} % @@ -4067,25 +10715,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kRadiusSun} -% |\kRadiusSun| is the mean radius of the Sun. +% \begin{macro}{\kCoulombNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kCoulombNumeric| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$). % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kRadiusSun}{% -\k@SI@short@RadiusSun} +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@SI@short@CoulombNumeric} \else -\DeclareRobustCommand {\kRadiusSun}{% -\k@SI@full@RadiusSun} +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@SI@full@CoulombNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kRadiusSun}{% -\k@cgs@short@RadiusSun} +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@cgs@short@CoulombNumeric} \else -\DeclareRobustCommand {\kRadiusSun}{% -\k@cgs@full@RadiusSun} +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@cgs@full@CoulombNumeric} \fi \fi % \end{macrocode} @@ -4094,22 +10743,19 @@ %\iffalse % %\fi -% -%\subsection{Energy, Power, and Luminosity} -% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@Rydberg} -% |\k@SI@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% \begin{macro}{\k@SI@short@VacuumPermittivity} +% |\k@SI@short@VacuumPermittivity| is the electric permittivity of the vacuum % in SI units with reduced precision. -% Source: Calculated +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@Rydberg}{% +\DeclareRobustCommand{\k@SI@short@VacuumPermittivity}{% \ensuremath{% -2.18% -\times 10^{-21}\Joule}} +8.85% +\times 10^{-12}\Farad\m^{-1}}} % \end{macrocode} % \end{macro} % @@ -4119,18 +10765,19 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@Rydberg} -% |\k@SI@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in SI units with full precision. -% Source: Calculated +% \begin{macro}{\k@SI@full@VacuumPermittivity} +% |\k@SI@full@VacuumPermittivity| is the electric permittivity of the vacuum in +% SI units with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@Rydberg}{% +\DeclareRobustCommand{\k@SI@full@VacuumPermittivity}{% \ensuremath{% -2.179\expandafter\physconst@decimalsseparator% -775\expandafter\physconst@decimalsseparator% -77% -\times 10^{-21}\Joule}} +8.854\expandafter\physconst@decimalsseparator% +187\expandafter\physconst@decimalsseparator% +812\expandafter\physconst@decimalsseparator% +8% +\times 10^{-12}\Farad\m^{-1}}} % \end{macrocode} % \end{macro} % @@ -4140,16 +10787,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@Rydberg} -% |\k@cgs@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% \begin{macro}{\k@cgs@short@VacuumPermittivity} +% |\k@cgs@short@VacuumPermittivity| is the electric permittivity of the vacuum % in cgs units with reduced precision. -% Source: Calculated +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@Rydberg}{% +\DeclareRobustCommand{\k@cgs@short@VacuumPermittivity}{% \ensuremath{% -2.18% -\times 10^{-14}\erg}} +7.96% +\times 10^{-2}}} % \end{macrocode} % \end{macro} % @@ -4159,58 +10806,19 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@Rydberg} -% |\k@cgs@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) +% \begin{macro}{\k@cgs@full@VacuumPermittivity} +% |\k@cgs@full@VacuumPermittivity| is the electric permittivity of the vacuum % in cgs units with full precision. -% Source: Calculated -% -% \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@Rydberg}{% -\ensuremath{% -2.179\expandafter\physconst@decimalsseparator% -775\expandafter\physconst@decimalsseparator% -77% -\times 10^{-14}\erg}} -% \end{macrocode} -% \end{macro} -% -%\iffalse -% -%\fi -%\iffalse -%<*package> -%\fi -% \begin{macro}{\k@eV@short@Rydberg} -% |\k@eV@short@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in eV with reduced precision. -% Source: Calculated -% -% \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@Rydberg}{% -\ensuremath{% -1.36% -\times 10^{-2}\eV}} -% \end{macrocode} -% \end{macro} -% -%\iffalse -% -%\fi -%\iffalse -%<*package> -%\fi -% \begin{macro}{\k@eV@full@Rydberg} -% |\k@eV@full@Rydberg| is the Rydberg energy (the binding energy of Hydrogen) -% in eV with full precision. -% Source: Calculated +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@Rydberg}{% +\DeclareRobustCommand{\k@cgs@full@VacuumPermittivity}{% \ensuremath{% -1.360\expandafter\physconst@decimalsseparator% -509\expandafter\physconst@decimalsseparator% -03% -\times 10^{-2}\eV}} +7.957\expandafter\physconst@decimalsseparator% +747\expandafter\physconst@decimalsseparator% +154\expandafter\physconst@decimalsseparator% +6% +\times 10^{-2}}} % \end{macrocode} % \end{macro} % @@ -4220,46 +10828,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kRydberg} -% |\kRydberg| is the Rydberg energy (the binding energy of Hydrogen). +% \begin{macro}{\kVacuumPermittivity} +% |\kVacuumPermittivity| is the electric permittivity of the vacuum. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kRydberg}{% -\k@SI@short@Rydberg} +\DeclareRobustCommand {\kVacuumPermittivity}{% +\k@SI@short@VacuumPermittivity} \else -\DeclareRobustCommand {\kRydberg}{% -\k@SI@full@Rydberg} +\DeclareRobustCommand {\kVacuumPermittivity}{% +\k@SI@full@VacuumPermittivity} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kRydberg}{% -\k@cgs@short@Rydberg} +\DeclareRobustCommand {\kVacuumPermittivity}{% +\k@cgs@short@VacuumPermittivity} \else -\DeclareRobustCommand {\kRydberg}{% -\k@cgs@full@Rydberg} -\fi +\DeclareRobustCommand {\kVacuumPermittivity}{% +\k@cgs@full@VacuumPermittivity} \fi -% \end{macrocode} -% \end{macro} -% -%\iffalse -% -%\fi -%\iffalse -%<*package> -%\fi -% \begin{macro}{\keVRydberg} -% |\keVRydberg| is the Rydberg energy (the binding energy of Hydrogen). -% -% \begin{macrocode} -\ifx\shortconst\undefined -\DeclareRobustCommand {\keVRydberg}{% -\k@eV@short@Rydberg} -\else -\DeclareRobustCommand {\keVRydberg}{% -\k@eV@full@Rydberg} \fi % \end{macrocode} % \end{macro} @@ -4270,16 +10858,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@LuminositySun} -% |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with -% reduced precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@SI@short@VacuumPermittivityNumeric} +% |\k@SI@short@VacuumPermittivityNumeric| is the electric permittivity of the vacuum +% in SI units with reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@LuminositySun}{% +\DeclareRobustCommand{\k@SI@short@VacuumPermittivityNumeric}{% \ensuremath{% -3.83% -\times 10^{26}\Watt}} +8.85e-12}} % \end{macrocode} % \end{macro} % @@ -4289,16 +10876,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@LuminositySun} -% |\k@SI@full@LuminositySun| is the luminosity of the Sun in SI units with full -% precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@SI@full@VacuumPermittivityNumeric} +% |\k@SI@full@VacuumPermittivityNumeric| is the electric permittivity of the vacuum in +% SI units with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@LuminositySun}{% +\DeclareRobustCommand{\k@SI@full@VacuumPermittivityNumeric}{% \ensuremath{% -3.828% -\times 10^{26}\Watt}} +8.8541878128e-12}} % \end{macrocode} % \end{macro} % @@ -4308,16 +10894,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@LuminositySun} -% |\k@cgs@short@LuminositySun| is the luminosity of the Sun in cgs units with -% reduced precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@cgs@short@VacuumPermittivityNumeric} +% |\k@cgs@short@VacuumPermittivityNumeric| is the electric permittivity of the vacuum +% in cgs units with reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@LuminositySun}{% +\DeclareRobustCommand{\k@cgs@short@VacuumPermittivityNumeric}{% \ensuremath{% -3.83% -\times 10^{33}\erg\Sec^{-1}}} +7.96e-02}} % \end{macrocode} % \end{macro} % @@ -4327,16 +10912,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@LuminositySun} -% |\k@cgs@full@LuminositySun| is the luminosity of the Sun in cgs units with -% full precision. -% Source: IAU~Resolution~B3~2015 +% \begin{macro}{\k@cgs@full@VacuumPermittivityNumeric} +% |\k@cgs@full@VacuumPermittivityNumeric| is the electric permittivity of the vacuum +% in cgs units with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@LuminositySun}{% +\DeclareRobustCommand{\k@cgs@full@VacuumPermittivityNumeric}{% \ensuremath{% -3.828% -\times 10^{33}\erg\Sec^{-1}}} +7.9577471546e-02}} % \end{macrocode} % \end{macro} % @@ -4346,25 +10930,25 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kLuminositySun} -% |\kLuminositySun| is the luminosity of the Sun. +% \begin{macro}{\kVacuumPermittivityNumeric} +% |\kVacuumPermittivityNumeric| is the electric permittivity of the vacuum. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kLuminositySun}{% -\k@SI@short@LuminositySun} +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@SI@short@VacuumPermittivityNumeric} \else -\DeclareRobustCommand {\kLuminositySun}{% -\k@SI@full@LuminositySun} +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@SI@full@VacuumPermittivityNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kLuminositySun}{% -\k@cgs@short@LuminositySun} +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@cgs@short@VacuumPermittivityNumeric} \else -\DeclareRobustCommand {\kLuminositySun}{% -\k@cgs@full@LuminositySun} +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@cgs@full@VacuumPermittivityNumeric} \fi \fi % \end{macrocode} @@ -4373,22 +10957,20 @@ %\iffalse % %\fi -% -%\subsection{Pressure} -% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@PressureAtmosphere} -% |\k@SI@short@PressureAtmosphere| is the standard atmospheric pressure in SI -% units with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@short@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@VacuumPermeability| is the magnetic permeability of the vacuum +% in SI units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@PressureAtmosphere}{% +\DeclareRobustCommand{\k@SI@short@VacuumPermeability}{% \ensuremath{% -1.01% -\times 10^{5}\Pa}} +1.26% +\times 10^{-6}\N\Amp^{-2}}} % \end{macrocode} % \end{macro} % @@ -4398,17 +10980,20 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@PressureAtmosphere} -% |\k@SI@full@PressureAtmosphere| is the standard atmospheric pressure in SI -% units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@VacuumPermeability| is the magnetic permeability of the vacuum in +% SI units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@PressureAtmosphere}{% +\DeclareRobustCommand{\k@SI@full@VacuumPermeability}{% \ensuremath{% -1.013\expandafter\physconst@decimalsseparator% -25% -\times 10^{5}\Pa}} +1.256\expandafter\physconst@decimalsseparator% +637\expandafter\physconst@decimalsseparator% +062\expandafter\physconst@decimalsseparator% +1% +\times 10^{-6}\N\Amp^{-2}}} % \end{macrocode} % \end{macro} % @@ -4418,15 +11003,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@PressureAtmosphere} -% |\k@cgs@short@PressureAtmosphere| is the standard atmospheric pressure in cgs -% units with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@VacuumPermeability| is the magnetic permeability of the vacuum +% in cgs units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@PressureAtmosphere}{% +\DeclareRobustCommand{\k@cgs@short@VacuumPermeability}{% \ensuremath{% -1.01\barP[m]}} +1.26% +\times 10^{1}}} % \end{macrocode} % \end{macro} % @@ -4436,16 +11023,20 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@PressureAtmosphere} -% |\k@cgs@full@PressureAtmosphere| is the standard atmospheric pressure in cgs -% units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@full@VacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@VacuumPermeability| is the magnetic permeability of the vacuum +% in cgs units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@PressureAtmosphere}{% +\DeclareRobustCommand{\k@cgs@full@VacuumPermeability}{% \ensuremath{% -1.013\expandafter\physconst@decimalsseparator% -25\barP[m]}} +1.256\expandafter\physconst@decimalsseparator% +637\expandafter\physconst@decimalsseparator% +061\expandafter\physconst@decimalsseparator% +4% +\times 10^{1}}} % \end{macrocode} % \end{macro} % @@ -4455,25 +11046,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kPressureAtmosphere} -% |\kPressureAtmosphere| is the standard atmospheric pressure. +% \begin{macro}{\kVacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\kVacuumPermeability| is the magnetic permeability of the vacuum. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kPressureAtmosphere}{% -\k@SI@short@PressureAtmosphere} +\DeclareRobustCommand {\kVacuumPermeability}{% +\k@SI@short@VacuumPermeability} \else -\DeclareRobustCommand {\kPressureAtmosphere}{% -\k@SI@full@PressureAtmosphere} +\DeclareRobustCommand {\kVacuumPermeability}{% +\k@SI@full@VacuumPermeability} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kPressureAtmosphere}{% -\k@cgs@short@PressureAtmosphere} +\DeclareRobustCommand {\kVacuumPermeability}{% +\k@cgs@short@VacuumPermeability} \else -\DeclareRobustCommand {\kPressureAtmosphere}{% -\k@cgs@full@PressureAtmosphere} +\DeclareRobustCommand {\kVacuumPermeability}{% +\k@cgs@full@VacuumPermeability} \fi \fi % \end{macrocode} @@ -4485,16 +11077,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@PressureStandard} -% |\k@SI@short@PressureStandard| is the standard atmospheric pressure in SI -% units with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@short@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum +% in SI units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@PressureStandard}{% +\DeclareRobustCommand{\k@SI@short@VacuumPermeabilityNumeric}{% \ensuremath{% -1.00% -\times 10^{5}\Pa}} +1.26e-06}} % \end{macrocode} % \end{macro} % @@ -4504,17 +11096,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@PressureStandard} -% |\k@SI@full@PressureStandard| is the standard atmospheric pressure in SI -% units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum in +% SI units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@PressureStandard}{% +\DeclareRobustCommand{\k@SI@full@VacuumPermeabilityNumeric}{% \ensuremath{% -1.000\expandafter\physconst@decimalsseparator% -00% -\times 10^{5}\Pa}} +1.2566370621e-06}} % \end{macrocode} % \end{macro} % @@ -4524,15 +11115,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@PressureStandard} -% |\k@cgs@short@PressureStandard| is the standard atmospheric pressure in cgs -% units with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum +% in cgs units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@PressureStandard}{% +\DeclareRobustCommand{\k@cgs@short@VacuumPermeabilityNumeric}{% \ensuremath{% -1.00\barP[m]}} +1.26e+01}} % \end{macrocode} % \end{macro} % @@ -4542,16 +11134,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@PressureStandard} -% |\k@cgs@full@PressureStandard| is the standard atmospheric pressure in cgs -% units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@full@VacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@VacuumPermeabilityNumeric| is the magnetic permeability of the vacuum +% in cgs units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@PressureStandard}{% +\DeclareRobustCommand{\k@cgs@full@VacuumPermeabilityNumeric}{% \ensuremath{% -1.000\expandafter\physconst@decimalsseparator% -00\barP[m]}} +1.2566370614e+01}} % \end{macrocode} % \end{macro} % @@ -4561,25 +11153,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kPressureStandard} -% |\kPressureStandard| is the standard atmospheric pressure. +% \begin{macro}{\kVacuumPermeabilityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\kVacuumPermeabilityNumeric| is the magnetic permeability of the vacuum. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kPressureStandard}{% -\k@SI@short@PressureStandard} +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@SI@short@VacuumPermeabilityNumeric} \else -\DeclareRobustCommand {\kPressureStandard}{% -\k@SI@full@PressureStandard} +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@SI@full@VacuumPermeabilityNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kPressureStandard}{% -\k@cgs@short@PressureStandard} +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@cgs@short@VacuumPermeabilityNumeric} \else -\DeclareRobustCommand {\kPressureStandard}{% -\k@cgs@full@PressureStandard} +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@cgs@full@VacuumPermeabilityNumeric} \fi \fi % \end{macrocode} @@ -4588,22 +11181,41 @@ %\iffalse % %\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@VacuumImpedance} +% |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with +% reduced precision. +% Source: CODATA~2018 % -%\subsection{Velocity, Speed and Acceleration} +% \begin{macrocode} +\DeclareRobustCommand{\k@short@VacuumImpedance}{% +\ensuremath{% +3.77% +\times 10^{2}\Ohm}} +% \end{macrocode} +% \end{macro} % %\iffalse +% +%\fi +%\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@SpeedLight} -% |\k@SI@short@SpeedLight| is the speed of light in SI units with reduced -% precision. -% Source: CODATA 2018 +% \begin{macro}{\k@full@VacuumImpedance} +% |\k@full@VacuumImpedance| is the characteristic impedance of the vacuum with +% full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@SpeedLight}{% +\DeclareRobustCommand{\k@full@VacuumImpedance}{% \ensuremath{% -3.00% -\times 10^{8}\m\Sec^{-1}}} +3.767\expandafter\physconst@decimalsseparator% +303\expandafter\physconst@decimalsseparator% +136\expandafter\physconst@decimalsseparator% +68% +\times 10^{2}\Ohm}} % \end{macrocode} % \end{macro} % @@ -4613,17 +11225,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@SpeedLight} -% |\k@SI@full@SpeedLight| is the speed of light in SI units with full precision. -% Source: CODATA 2018 +% \begin{macro}{\kVacuumImpedance} +% |\kVacuumImpedance| is the characteristic impedance of the vacuum. % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@SpeedLight}{% -\ensuremath{% -2.997\expandafter\physconst@decimalsseparator% -924\expandafter\physconst@decimalsseparator% -58% -\times 10^{8}\m\Sec^{-1}}} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kVacuumImpedance}{% +\k@short@VacuumImpedance} +\else +\DeclareRobustCommand {\kVacuumImpedance}{% +\k@full@VacuumImpedance} +\fi % \end{macrocode} % \end{macro} % @@ -4633,16 +11245,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@SpeedLight} -% |\k@cgs@short@SpeedLight| is the speed of light in cgs units with reduced -% precision. -% Source: CODATA 2018 +% \begin{macro}{\k@short@VacuumImpedanceNumeric} +% |\k@short@VacuumImpedanceNumeric| is the characteristic impedance of the vacuum with +% reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@SpeedLight}{% +\DeclareRobustCommand{\k@short@VacuumImpedanceNumeric}{% \ensuremath{% -3.00% -\times 10^{10}\cm\Sec^{-1}}} +3.77e+02}} % \end{macrocode} % \end{macro} % @@ -4652,18 +11263,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@SpeedLight} -% |\k@cgs@full@SpeedLight| is the speed of light in cgs units with full -% precision. -% Source: CODATA 2018 +% \begin{macro}{\k@full@VacuumImpedanceNumeric} +% |\k@full@VacuumImpedanceNumeric| is the characteristic impedance of the vacuum with +% full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@SpeedLight}{% +\DeclareRobustCommand{\k@full@VacuumImpedanceNumeric}{% \ensuremath{% -2.997\expandafter\physconst@decimalsseparator% -924\expandafter\physconst@decimalsseparator% -58% -\times 10^{10}\cm\Sec^{-1}}} +3.76730313668e+02}} % \end{macrocode} % \end{macro} % @@ -4673,26 +11281,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kSpeedLight} -% |\kSpeedLight| is the speed of light. +% \begin{macro}{\kVacuumImpedanceNumeric} +% |\kVacuumImpedanceNumeric| is the characteristic impedance of the vacuum. % % \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kSpeedLight}{% -\k@SI@short@SpeedLight} -\else -\DeclareRobustCommand {\kSpeedLight}{% -\k@SI@full@SpeedLight} -\fi -\else \ifx\shortconst\undefined -\DeclareRobustCommand {\kSpeedLight}{% -\k@cgs@short@SpeedLight} +\DeclareRobustCommand {\kVacuumImpedanceNumeric}{% +\k@short@VacuumImpedanceNumeric} \else -\DeclareRobustCommand {\kSpeedLight}{% -\k@cgs@full@SpeedLight} -\fi +\DeclareRobustCommand {\kVacuumImpedanceNumeric}{% +\k@full@VacuumImpedanceNumeric} \fi % \end{macrocode} % \end{macro} @@ -4703,16 +11301,55 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@AccelGravity} -% |\k@SI@short@AccelGravity| is the accelertion due to gravity at the surface -% of the Earth in SI units with reduced precision. -% Source: CODATA 2018 +% \begin{macro}{\k@SI@short@Boltzmann} +% |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@Boltzmann}{% +\ensuremath{% +1.38% +\times 10^{-23}\J\K^{-1}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@Boltzmann} +% |\k@SI@full@Boltzmann| is the Boltzmann constant in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@Boltzmann}{% +\ensuremath{% +1.380\expandafter\physconst@decimalsseparator% +649% +\times 10^{-23}\J\K^{-1}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@Boltzmann} +% |\k@cgs@short@Boltzmann| is the Boltzmann constant in cgs units with reduced +% precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@AccelGravity}{% +\DeclareRobustCommand{\k@cgs@short@Boltzmann}{% \ensuremath{% -6.67% -\times 10^{-11}\N\kg^{-2}\m^2}} +1.38% +\times 10^{-16}\erg\K^{-1}}} % \end{macrocode} % \end{macro} % @@ -4722,17 +11359,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@AccelGravity} -% |\k@SI@full@AccelGravity| is the accelertion due to gravity at the surface of -% the Earth in SI units with full precision. -% Source: CODATA 2018 +% \begin{macro}{\k@cgs@full@Boltzmann} +% |\k@cgs@full@Boltzmann| is the Boltzmann constant in cgs units with full +% precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@AccelGravity}{% +\DeclareRobustCommand{\k@cgs@full@Boltzmann}{% \ensuremath{% -6.674\expandafter\physconst@decimalsseparator% -30% -\times 10^{-11}\N\kg^{-2}\m^2}} +1.380\expandafter\physconst@decimalsseparator% +649% +\times 10^{-16}\erg\K^{-1}}} % \end{macrocode} % \end{macro} % @@ -4742,16 +11379,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@AccelGravity} -% |\k@cgs@short@AccelGravity| is the accelertion due to gravity at the surface -% of the Earth in cgs units with reduced precision. -% Source: CODATA 2018 +% \begin{macro}{\k@eV@short@Boltzmann} +% |\k@eV@short@Boltzmann| is the Boltzmann constant in eV with reduced +% precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@AccelGravity}{% +\DeclareRobustCommand{\k@eV@short@Boltzmann}{% \ensuremath{% -6.67% -\times 10^{-8}\dyne\gm^{-2}\cm^2}} +8.62% +\times 10^{-5}\eV\K^{-1}}} % \end{macrocode} % \end{macro} % @@ -4761,17 +11398,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@AccelGravity} -% |\k@cgs@full@AccelGravity| is the accelertion due to gravity at the surface -% of the Earth in cgs units with full precision. -% Source: CODATA 2018 +% \begin{macro}{\k@eV@full@Boltzmann} +% |\k@eV@full@Boltzmann| is the Boltzmann constant in eV with full precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@AccelGravity}{% +\DeclareRobustCommand{\k@eV@full@Boltzmann}{% \ensuremath{% -6.674\expandafter\physconst@decimalsseparator% -30% -\times 10^{-8}\dyne\gm^{-2}\cm^2}} +8.617\expandafter\physconst@decimalsseparator% +333% +\times 10^{-5}\eV\K^{-1}}} % \end{macrocode} % \end{macro} % @@ -4781,26 +11417,25 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kAccelGravity} -% |\kAccelGravity| is the accelertion due to gravity at the surface of the -% Earth. +% \begin{macro}{\kBoltzmann} +% |\kBoltzmann| is the Boltzmann constant. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kAccelGravity}{% -\k@SI@short@AccelGravity} +\DeclareRobustCommand {\kBoltzmann}{% +\k@SI@short@Boltzmann} \else -\DeclareRobustCommand {\kAccelGravity}{% -\k@SI@full@AccelGravity} +\DeclareRobustCommand {\kBoltzmann}{% +\k@SI@full@Boltzmann} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kAccelGravity}{% -\k@cgs@short@AccelGravity} +\DeclareRobustCommand {\kBoltzmann}{% +\k@cgs@short@Boltzmann} \else -\DeclareRobustCommand {\kAccelGravity}{% -\k@cgs@full@AccelGravity} +\DeclareRobustCommand {\kBoltzmann}{% +\k@cgs@full@Boltzmann} \fi \fi % \end{macrocode} @@ -4809,22 +11444,20 @@ %\iffalse % %\fi -% -%\subsection{Other Constants} -% %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@Coulomb} -% |\k@SI@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in -% SI units with reduced precision. -% Source: Calculated +% \begin{macro}{\keVBoltzmann} +% |\keVBoltzmann| is the Boltzmann constant. % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@Coulomb}{% -\ensuremath{% -8.99% -\times 10^{13}\N\m^2\Coulomb^{-2}}} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVBoltzmann}{% +\k@eV@short@Boltzmann} +\else +\DeclareRobustCommand {\keVBoltzmann}{% +\k@eV@full@Boltzmann} +\fi % \end{macrocode} % \end{macro} % @@ -4834,18 +11467,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@Coulomb} -% |\k@SI@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in -% SI units with full precision. -% Source: Calculated +% \begin{macro}{\k@SI@short@BoltzmannNumeric} +% |\k@SI@short@BoltzmannNumeric| is the Boltzmann constant in SI units with reduced +% precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@Coulomb}{% +\DeclareRobustCommand{\k@SI@short@BoltzmannNumeric}{% \ensuremath{% -8.987\expandafter\physconst@decimalsseparator% -551\expandafter\physconst@decimalsseparator% -79% -\times 10^{13}\N\m^2\Coulomb^{-2}}} +1.38e-23}} % \end{macrocode} % \end{macro} % @@ -4855,15 +11485,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@Coulomb} -% |\k@cgs@short@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) -% in cgs units with reduced precision. -% Source: Calculated +% \begin{macro}{\k@SI@full@BoltzmannNumeric} +% |\k@SI@full@BoltzmannNumeric| is the Boltzmann constant in SI units with full +% precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@Coulomb}{% +\DeclareRobustCommand{\k@SI@full@BoltzmannNumeric}{% \ensuremath{% -1.00}} +1.380649e-23}} % \end{macrocode} % \end{macro} % @@ -4873,47 +11503,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@Coulomb} -% |\k@cgs@full@Coulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$) in -% cgs units with full precision. -% Source: Calculated +% \begin{macro}{\k@cgs@short@BoltzmannNumeric} +% |\k@cgs@short@BoltzmannNumeric| is the Boltzmann constant in cgs units with reduced +% precision. +% Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@Coulomb}{% +\DeclareRobustCommand{\k@cgs@short@BoltzmannNumeric}{% \ensuremath{% -1.000\expandafter\physconst@decimalsseparator% -000\expandafter\physconst@decimalsseparator% -00}} -% \end{macrocode} -% \end{macro} -% -%\iffalse -% -%\fi -%\iffalse -%<*package> -%\fi -% \begin{macro}{\kCoulomb} -% |\kCoulomb| is the Coulomb constant ($\frac{1}{4\pi\epsilon_0}$). -% -% \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kCoulomb}{% -\k@SI@short@Coulomb} -\else -\DeclareRobustCommand {\kCoulomb}{% -\k@SI@full@Coulomb} -\fi -\else -\ifx\shortconst\undefined -\DeclareRobustCommand {\kCoulomb}{% -\k@cgs@short@Coulomb} -\else -\DeclareRobustCommand {\kCoulomb}{% -\k@cgs@full@Coulomb} -\fi -\fi +1.38e-16}} % \end{macrocode} % \end{macro} % @@ -4923,16 +11521,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@VacuumPermittivity} -% |\k@SI@short@VacuumPermittivity| is the electric permittivity of the vacuum -% in SI units with reduced precision. +% \begin{macro}{\k@cgs@full@BoltzmannNumeric} +% |\k@cgs@full@BoltzmannNumeric| is the Boltzmann constant in cgs units with full +% precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@VacuumPermittivity}{% +\DeclareRobustCommand{\k@cgs@full@BoltzmannNumeric}{% \ensuremath{% -8.85% -\times 10^{-12}\Farad\m^{-1}}} +1.380649e-16}} % \end{macrocode} % \end{macro} % @@ -4942,19 +11539,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@VacuumPermittivity} -% |\k@SI@full@VacuumPermittivity| is the electric permittivity of the vacuum in -% SI units with full precision. +% \begin{macro}{\k@eV@short@BoltzmannNumeric} +% |\k@eV@short@BoltzmannNumeric| is the Boltzmann constant in eV with reduced +% precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@VacuumPermittivity}{% +\DeclareRobustCommand{\k@eV@short@BoltzmannNumeric}{% \ensuremath{% -8.854\expandafter\physconst@decimalsseparator% -187\expandafter\physconst@decimalsseparator% -812\expandafter\physconst@decimalsseparator% -8% -\times 10^{-12}\Farad\m^{-1}}} +8.62e-05}} % \end{macrocode} % \end{macro} % @@ -4964,16 +11557,14 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@VacuumPermittivity} -% |\k@cgs@short@VacuumPermittivity| is the electric permittivity of the vacuum -% in cgs units with reduced precision. +% \begin{macro}{\k@eV@full@BoltzmannNumeric} +% |\k@eV@full@BoltzmannNumeric| is the Boltzmann constant in eV with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@VacuumPermittivity}{% +\DeclareRobustCommand{\k@eV@full@BoltzmannNumeric}{% \ensuremath{% -7.96% -\times 10^{-2}}} +8.617333e-05}} % \end{macrocode} % \end{macro} % @@ -4983,19 +11574,27 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@VacuumPermittivity} -% |\k@cgs@full@VacuumPermittivity| is the electric permittivity of the vacuum -% in cgs units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\kBoltzmannNumeric} +% |\kBoltzmannNumeric| is the Boltzmann constant. % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@VacuumPermittivity}{% -\ensuremath{% -7.957\expandafter\physconst@decimalsseparator% -747\expandafter\physconst@decimalsseparator% -154\expandafter\physconst@decimalsseparator% -6% -\times 10^{-2}}} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kBoltzmannNumeric}{% +\k@SI@short@BoltzmannNumeric} +\else +\DeclareRobustCommand {\kBoltzmannNumeric}{% +\k@SI@full@BoltzmannNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kBoltzmannNumeric}{% +\k@cgs@short@BoltzmannNumeric} +\else +\DeclareRobustCommand {\kBoltzmannNumeric}{% +\k@cgs@full@BoltzmannNumeric} +\fi +\fi % \end{macrocode} % \end{macro} % @@ -5005,26 +11604,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kVacuumPermittivity} -% |\kVacuumPermittivity| is the electric permittivity of the vacuum. +% \begin{macro}{\keVBoltzmannNumeric} +% |\keVBoltzmannNumeric| is the Boltzmann constant. % % \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kVacuumPermittivity}{% -\k@SI@short@VacuumPermittivity} -\else -\DeclareRobustCommand {\kVacuumPermittivity}{% -\k@SI@full@VacuumPermittivity} -\fi -\else \ifx\shortconst\undefined -\DeclareRobustCommand {\kVacuumPermittivity}{% -\k@cgs@short@VacuumPermittivity} +\DeclareRobustCommand {\keVBoltzmannNumeric}{% +\k@eV@short@BoltzmannNumeric} \else -\DeclareRobustCommand {\kVacuumPermittivity}{% -\k@cgs@full@VacuumPermittivity} -\fi +\DeclareRobustCommand {\keVBoltzmannNumeric}{% +\k@eV@full@BoltzmannNumeric} \fi % \end{macrocode} % \end{macro} @@ -5035,16 +11624,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@VacuumPermeability} -% |\k@SI@short@VacuumPermeability| is the magnetic permeability of the vacuum -% in SI units with reduced precision. +% \begin{macro}{\k@SI@short@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@Planck| is the Planck constant in SI units with reduced +% precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@VacuumPermeability}{% +\DeclareRobustCommand{\k@SI@short@Planck}{% \ensuremath{% -8.85% -\times 10^{-12}\N\Amp^{-2}}} +6.63% +\times 10^{-34}\J\Sec}} % \end{macrocode} % \end{macro} % @@ -5054,19 +11644,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@VacuumPermeability} -% |\k@SI@full@VacuumPermeability| is the magnetic permeability of the vacuum in -% SI units with full precision. +% \begin{macro}{\k@SI@full@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@Planck| is the Planck constant in SI units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@VacuumPermeability}{% +\DeclareRobustCommand{\k@SI@full@Planck}{% \ensuremath{% -8.854\expandafter\physconst@decimalsseparator% -187\expandafter\physconst@decimalsseparator% -812\expandafter\physconst@decimalsseparator% -8% -\times 10^{-12}\N\Amp^{-2}}} +6.626\expandafter\physconst@decimalsseparator% +070\expandafter\physconst@decimalsseparator% +15% +\times 10^{-34}\J\Sec}} % \end{macrocode} % \end{macro} % @@ -5076,16 +11665,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@VacuumPermeability} -% |\k@cgs@short@VacuumPermeability| is the magnetic permeability of the vacuum -% in cgs units with reduced precision. +% \begin{macro}{\k@cgs@short@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@Planck| is the Planck constant in cgs units with reduced +% precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@VacuumPermeability}{% +\DeclareRobustCommand{\k@cgs@short@Planck}{% \ensuremath{% -1.26% -\times 10^{1}}} +6.63% +\times 10^{-27}\erg\Sec}} % \end{macrocode} % \end{macro} % @@ -5095,19 +11685,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@VacuumPermeability} -% |\k@cgs@full@VacuumPermeability| is the magnetic permeability of the vacuum -% in cgs units with full precision. +% \begin{macro}{\k@cgs@full@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@Planck| is the Planck constant in cgs units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@VacuumPermeability}{% +\DeclareRobustCommand{\k@cgs@full@Planck}{% \ensuremath{% -1.256\expandafter\physconst@decimalsseparator% -637\expandafter\physconst@decimalsseparator% -061\expandafter\physconst@decimalsseparator% -4% -\times 10^{1}}} +6.626\expandafter\physconst@decimalsseparator% +070\expandafter\physconst@decimalsseparator% +15% +\times 10^{-27}\erg\Sec}} % \end{macrocode} % \end{macro} % @@ -5117,27 +11706,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kVacuumPermeability} -% |\kVacuumPermeability| is the magnetic permeability of the vacuum. +% \begin{macro}{\k@eV@short@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@Planck| is the Planck constant in eV with reduced precision. +% Source: CODATA~2018 % % \begin{macrocode} -\ifx\cgsunits\undefined -\ifx\shortconst\undefined -\DeclareRobustCommand {\kVacuumPermeability}{% -\k@SI@short@VacuumPermeability} -\else -\DeclareRobustCommand {\kVacuumPermeability}{% -\k@SI@full@VacuumPermeability} -\fi -\else -\ifx\shortconst\undefined -\DeclareRobustCommand {\kVacuumPermeability}{% -\k@cgs@short@VacuumPermeability} -\else -\DeclareRobustCommand {\kVacuumPermeability}{% -\k@cgs@full@VacuumPermeability} -\fi -\fi +\DeclareRobustCommand{\k@eV@short@Planck}{% +\ensuremath{% +4.14% +\times 10^{-15}\eV\Sec}} % \end{macrocode} % \end{macro} % @@ -5147,16 +11725,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@short@VacuumImpedance} -% |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with -% reduced precision. +% \begin{macro}{\k@eV@full@Planck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@Planck| is the Planck constant in eV with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@short@VacuumImpedance}{% +\DeclareRobustCommand{\k@eV@full@Planck}{% \ensuremath{% -3.77% -\times 10^{2}\Ohm}} +4.135\expandafter\physconst@decimalsseparator% +667\expandafter\physconst@decimalsseparator% +70% +\times 10^{-15}\eV\Sec}} % \end{macrocode} % \end{macro} % @@ -5166,19 +11746,28 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@full@VacuumImpedance} -% |\k@full@VacuumImpedance| is the characteristic impedance of the vacuum with -% full precision. -% Source: CODATA~2018 +% \begin{macro}{\kPlanck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kPlanck| is the Planck constant. % % \begin{macrocode} -\DeclareRobustCommand{\k@full@VacuumImpedance}{% -\ensuremath{% -3.767\expandafter\physconst@decimalsseparator% -303\expandafter\physconst@decimalsseparator% -136\expandafter\physconst@decimalsseparator% -68% -\times 10^{2}\Ohm}} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPlanck}{% +\k@SI@short@Planck} +\else +\DeclareRobustCommand {\kPlanck}{% +\k@SI@full@Planck} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPlanck}{% +\k@cgs@short@Planck} +\else +\DeclareRobustCommand {\kPlanck}{% +\k@cgs@full@Planck} +\fi +\fi % \end{macrocode} % \end{macro} % @@ -5188,16 +11777,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kVacuumImpedance} -% |\kVacuumImpedance| is the characteristic impedance of the vacuum. +% \begin{macro}{\keVPlanck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\keVPlanck| is the Planck constant. % % \begin{macrocode} \ifx\shortconst\undefined -\DeclareRobustCommand {\kVacuumImpedance}{% -\k@short@VacuumImpedance} +\DeclareRobustCommand {\keVPlanck}{% +\k@eV@short@Planck} \else -\DeclareRobustCommand {\kVacuumImpedance}{% -\k@full@VacuumImpedance} +\DeclareRobustCommand {\keVPlanck}{% +\k@eV@full@Planck} \fi % \end{macrocode} % \end{macro} @@ -5208,16 +11798,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@Boltzmann} -% |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced +% \begin{macro}{\k@SI@short@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@PlanckNumeric| is the Planck constant in SI units with reduced % precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@Boltzmann}{% +\DeclareRobustCommand{\k@SI@short@PlanckNumeric}{% \ensuremath{% -1.38% -\times 10^{-23}\J\K^{-1}}} +6.63e-34}} % \end{macrocode} % \end{macro} % @@ -5227,17 +11817,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@Boltzmann} -% |\k@SI@full@Boltzmann| is the Boltzmann constant in SI units with full -% precision. +% \begin{macro}{\k@SI@full@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@PlanckNumeric| is the Planck constant in SI units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@Boltzmann}{% +\DeclareRobustCommand{\k@SI@full@PlanckNumeric}{% \ensuremath{% -1.380\expandafter\physconst@decimalsseparator% -649% -\times 10^{-23}\J\K^{-1}}} +6.62607015e-34}} % \end{macrocode} % \end{macro} % @@ -5247,16 +11835,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@Boltzmann} -% |\k@cgs@short@Boltzmann| is the Boltzmann constant in cgs units with reduced +% \begin{macro}{\k@cgs@short@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@PlanckNumeric| is the Planck constant in cgs units with reduced % precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@Boltzmann}{% +\DeclareRobustCommand{\k@cgs@short@PlanckNumeric}{% \ensuremath{% -1.38% -\times 10^{-16}\erg\K^{-1}}} +6.63e-27}} % \end{macrocode} % \end{macro} % @@ -5266,17 +11854,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@Boltzmann} -% |\k@cgs@full@Boltzmann| is the Boltzmann constant in cgs units with full -% precision. +% \begin{macro}{\k@cgs@full@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@PlanckNumeric| is the Planck constant in cgs units with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@Boltzmann}{% +\DeclareRobustCommand{\k@cgs@full@PlanckNumeric}{% \ensuremath{% -1.380\expandafter\physconst@decimalsseparator% -649% -\times 10^{-16}\erg\K^{-1}}} +6.62607015e-27}} % \end{macrocode} % \end{macro} % @@ -5286,16 +11872,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@Boltzmann} -% |\k@eV@short@Boltzmann| is the Boltzmann constant in eV with reduced -% precision. +% \begin{macro}{\k@eV@short@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@PlanckNumeric| is the Planck constant in eV with reduced precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@Boltzmann}{% +\DeclareRobustCommand{\k@eV@short@PlanckNumeric}{% \ensuremath{% -8.62% -\times 10^{-5}\eV\K^{-1}}} +4.14e-15}} % \end{macrocode} % \end{macro} % @@ -5305,16 +11890,15 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@Boltzmann} -% |\k@eV@full@Boltzmann| is the Boltzmann constant in eV with full precision. +% \begin{macro}{\k@eV@full@PlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@PlanckNumeric| is the Planck constant in eV with full precision. % Source: CODATA~2018 % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@Boltzmann}{% +\DeclareRobustCommand{\k@eV@full@PlanckNumeric}{% \ensuremath{% -8.617\expandafter\physconst@decimalsseparator% -333% -\times 10^{-5}\eV\K^{-1}}} +4.13566770e-15}} % \end{macrocode} % \end{macro} % @@ -5324,25 +11908,26 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kBoltzmann} -% |\kBoltzmann| is the Boltzmann constant. +% \begin{macro}{\kPlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kPlanckNumeric| is the Planck constant. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kBoltzmann}{% -\k@SI@short@Boltzmann} +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@SI@short@PlanckNumeric} \else -\DeclareRobustCommand {\kBoltzmann}{% -\k@SI@full@Boltzmann} +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@SI@full@PlanckNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kBoltzmann}{% -\k@cgs@short@Boltzmann} +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@cgs@short@PlanckNumeric} \else -\DeclareRobustCommand {\kBoltzmann}{% -\k@cgs@full@Boltzmann} +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@cgs@full@PlanckNumeric} \fi \fi % \end{macrocode} @@ -5354,16 +11939,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\keVBoltzmann} -% |\keVBoltzmann| is the Boltzmann constant. +% \begin{macro}{\keVPlanckNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\keVPlanckNumeric| is the Planck constant. % % \begin{macrocode} \ifx\shortconst\undefined -\DeclareRobustCommand {\keVBoltzmann}{% -\k@eV@short@Boltzmann} +\DeclareRobustCommand {\keVPlanckNumeric}{% +\k@eV@short@PlanckNumeric} \else -\DeclareRobustCommand {\keVBoltzmann}{% -\k@eV@full@Boltzmann} +\DeclareRobustCommand {\keVPlanckNumeric}{% +\k@eV@full@PlanckNumeric} \fi % \end{macrocode} % \end{macro} @@ -5374,15 +11960,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@Planck} -% |\k@SI@short@Planck| is the Planck constant in SI units with reduced -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@short@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@Planck}{% +\DeclareRobustCommand{\k@SI@short@PlanckReduced}{% \ensuremath{% -6.63% +1.05% \times 10^{-34}\J\Sec}} % \end{macrocode} % \end{macro} @@ -5393,16 +11980,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@Planck} -% |\k@SI@full@Planck| is the Planck constant in SI units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@SI@full@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in SI units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@Planck}{% +\DeclareRobustCommand{\k@SI@full@PlanckReduced}{% \ensuremath{% -6.626\expandafter\physconst@decimalsseparator% -070\expandafter\physconst@decimalsseparator% -15% +1.054\expandafter\physconst@decimalsseparator% +571\expandafter\physconst@decimalsseparator% +82% \times 10^{-34}\J\Sec}} % \end{macrocode} % \end{macro} @@ -5413,15 +12002,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@Planck} -% |\k@cgs@short@Planck| is the Planck constant in cgs units with reduced -% precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@short@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@Planck}{% +\DeclareRobustCommand{\k@cgs@short@PlanckReduced}{% \ensuremath{% -6.63% +1.05% \times 10^{-27}\erg\Sec}} % \end{macrocode} % \end{macro} @@ -5432,16 +12022,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@Planck} -% |\k@cgs@full@Planck| is the Planck constant in cgs units with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@cgs@full@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@Planck}{% +\DeclareRobustCommand{\k@cgs@full@PlanckReduced}{% \ensuremath{% -6.626\expandafter\physconst@decimalsseparator% -070\expandafter\physconst@decimalsseparator% -15% +1.054\expandafter\physconst@decimalsseparator% +571\expandafter\physconst@decimalsseparator% +82% \times 10^{-27}\erg\Sec}} % \end{macrocode} % \end{macro} @@ -5452,15 +12044,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@Planck} -% |\k@eV@short@Planck| is the Planck constant in eV with reduced precision. -% Source: CODATA~2018 +% \begin{macro}{\k@eV@short@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@Planck}{% +\DeclareRobustCommand{\k@eV@short@PlanckReduced}{% \ensuremath{% -4.14% -\times 10^{-15}\eV\Sec}} +6.58% +\times 10^{-16}\eV\Sec}} % \end{macrocode} % \end{macro} % @@ -5470,17 +12064,19 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@Planck} -% |\k@eV@full@Planck| is the Planck constant in eV with full precision. -% Source: CODATA~2018 +% \begin{macro}{\k@eV@full@PlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@PlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$ in eV with full precision. +% Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@Planck}{% +\DeclareRobustCommand{\k@eV@full@PlanckReduced}{% \ensuremath{% -4.135\expandafter\physconst@decimalsseparator% -667\expandafter\physconst@decimalsseparator% -70% -\times 10^{-15}\eV\Sec}} +6.582\expandafter\physconst@decimalsseparator% +119\expandafter\physconst@decimalsseparator% +57% +\times 10^{-16}\eV\Sec}} % \end{macrocode} % \end{macro} % @@ -5490,25 +12086,27 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kPlanck} -% |\kPlanck| is the Planck constant. +% \begin{macro}{\kPlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kPlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kPlanck}{% -\k@SI@short@Planck} +\DeclareRobustCommand {\kPlanckReduced}{% +\k@SI@short@PlanckReduced} \else -\DeclareRobustCommand {\kPlanck}{% -\k@SI@full@Planck} +\DeclareRobustCommand {\kPlanckReduced}{% +\k@SI@full@PlanckReduced} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kPlanck}{% -\k@cgs@short@Planck} +\DeclareRobustCommand {\kPlanckReduced}{% +\k@cgs@short@PlanckReduced} \else -\DeclareRobustCommand {\kPlanck}{% -\k@cgs@full@Planck} +\DeclareRobustCommand {\kPlanckReduced}{% +\k@cgs@full@PlanckReduced} \fi \fi % \end{macrocode} @@ -5520,16 +12118,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\keVPlanck} -% |\keVPlanck| is the Planck constant. +% \begin{macro}{\keVPlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\keVPlanckReduced| is the Reduced Planck constant +% $\left(\frac{h}{2\pi}\right)$. % % \begin{macrocode} \ifx\shortconst\undefined -\DeclareRobustCommand {\keVPlanck}{% -\k@eV@short@Planck} +\DeclareRobustCommand {\keVPlanckReduced}{% +\k@eV@short@PlanckReduced} \else -\DeclareRobustCommand {\keVPlanck}{% -\k@eV@full@Planck} +\DeclareRobustCommand {\keVPlanckReduced}{% +\k@eV@full@PlanckReduced} \fi % \end{macrocode} % \end{macro} @@ -5540,16 +12140,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@PlanckReduced} -% |\k@SI@short@PlanckReduced| is the Reduced Planck constant +% \begin{macro}{\k@SI@short@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@PlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$ in SI units with reduced precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@PlanckReduced}{% +\DeclareRobustCommand{\k@SI@short@PlanckReducedNumeric}{% \ensuremath{% -1.05% -\times 10^{-34}\J\Sec}} +1.05e-34}} % \end{macrocode} % \end{macro} % @@ -5559,18 +12159,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@PlanckReduced} -% |\k@SI@full@PlanckReduced| is the Reduced Planck constant +% \begin{macro}{\k@SI@full@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@PlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$ in SI units with full precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@PlanckReduced}{% +\DeclareRobustCommand{\k@SI@full@PlanckReducedNumeric}{% \ensuremath{% -1.054\expandafter\physconst@decimalsseparator% -571\expandafter\physconst@decimalsseparator% -82% -\times 10^{-34}\J\Sec}} +1.05457182e-34}} % \end{macrocode} % \end{macro} % @@ -5580,16 +12178,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@PlanckReduced} -% |\k@cgs@short@PlanckReduced| is the Reduced Planck constant +% \begin{macro}{\k@cgs@short@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@PlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$ in cgs units with reduced precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@PlanckReduced}{% +\DeclareRobustCommand{\k@cgs@short@PlanckReducedNumeric}{% \ensuremath{% -1.05% -\times 10^{-27}\erg\Sec}} +1.05e-27}} % \end{macrocode} % \end{macro} % @@ -5599,18 +12197,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@PlanckReduced} -% |\k@cgs@full@PlanckReduced| is the Reduced Planck constant +% \begin{macro}{\k@cgs@full@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@PlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$ in cgs units with full precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@PlanckReduced}{% +\DeclareRobustCommand{\k@cgs@full@PlanckReducedNumeric}{% \ensuremath{% -1.054\expandafter\physconst@decimalsseparator% -571\expandafter\physconst@decimalsseparator% -82% -\times 10^{-27}\erg\Sec}} +1.05457182e-27}} % \end{macrocode} % \end{macro} % @@ -5620,16 +12216,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@short@PlanckReduced} -% |\k@eV@short@PlanckReduced| is the Reduced Planck constant +% \begin{macro}{\k@eV@short@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@short@PlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$ in eV with reduced precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@short@PlanckReduced}{% +\DeclareRobustCommand{\k@eV@short@PlanckReducedNumeric}{% \ensuremath{% -6.58% -\times 10^{-16}\eV\Sec}} +6.58e-16}} % \end{macrocode} % \end{macro} % @@ -5639,18 +12235,16 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@eV@full@PlanckReduced} -% |\k@eV@full@PlanckReduced| is the Reduced Planck constant +% \begin{macro}{\k@eV@full@PlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@eV@full@PlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$ in eV with full precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@eV@full@PlanckReduced}{% +\DeclareRobustCommand{\k@eV@full@PlanckReducedNumeric}{% \ensuremath{% -6.582\expandafter\physconst@decimalsseparator% -119\expandafter\physconst@decimalsseparator% -57% -\times 10^{-16}\eV\Sec}} +6.58211957e-16}} % \end{macrocode} % \end{macro} % @@ -5660,26 +12254,27 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kPlanckReduced} -% |\kPlanckReduced| is the Reduced Planck constant +% \begin{macro}{\kPlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kPlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kPlanckReduced}{% -\k@SI@short@PlanckReduced} +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@SI@short@PlanckReducedNumeric} \else -\DeclareRobustCommand {\kPlanckReduced}{% -\k@SI@full@PlanckReduced} +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@SI@full@PlanckReducedNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kPlanckReduced}{% -\k@cgs@short@PlanckReduced} +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@cgs@short@PlanckReducedNumeric} \else -\DeclareRobustCommand {\kPlanckReduced}{% -\k@cgs@full@PlanckReduced} +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@cgs@full@PlanckReducedNumeric} \fi \fi % \end{macrocode} @@ -5691,17 +12286,18 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\keVPlanckReduced} -% |\keVPlanckReduced| is the Reduced Planck constant +% \begin{macro}{\keVPlanckReducedNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\keVPlanckReducedNumeric| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$. % % \begin{macrocode} \ifx\shortconst\undefined -\DeclareRobustCommand {\keVPlanckReduced}{% -\k@eV@short@PlanckReduced} +\DeclareRobustCommand {\keVPlanckReducedNumeric}{% +\k@eV@short@PlanckReducedNumeric} \else -\DeclareRobustCommand {\keVPlanckReduced}{% -\k@eV@full@PlanckReduced} +\DeclareRobustCommand {\keVPlanckReducedNumeric}{% +\k@eV@full@PlanckReducedNumeric} \fi % \end{macrocode} % \end{macro} @@ -5713,6 +12309,7 @@ %<*package> %\fi % \begin{macro}{\k@SI@short@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\k@SI@short@Gravity| is Newton's gravitational constant in SI units with % reduced precision. % Source: CODATA~2018 @@ -5721,7 +12318,7 @@ \DeclareRobustCommand{\k@SI@short@Gravity}{% \ensuremath{% 6.67% -\times 10^{-15}\N\kg^{-2}\m^2}} +\times 10^{-11}\N\kg^{-2}\m^2}} % \end{macrocode} % \end{macro} % @@ -5732,6 +12329,7 @@ %<*package> %\fi % \begin{macro}{\k@SI@full@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\k@SI@full@Gravity| is Newton's gravitational constant in SI units with full % precision. % Source: CODATA~2018 @@ -5741,7 +12339,7 @@ \ensuremath{% 6.674\expandafter\physconst@decimalsseparator% 30% -\times 10^{-15}\N\kg^{-2}\m^2}} +\times 10^{-11}\N\kg^{-2}\m^2}} % \end{macrocode} % \end{macro} % @@ -5752,6 +12350,7 @@ %<*package> %\fi % \begin{macro}{\k@cgs@short@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\k@cgs@short@Gravity| is Newton's gravitational constant in cgs units with % reduced precision. % Source: CODATA~2018 @@ -5771,6 +12370,7 @@ %<*package> %\fi % \begin{macro}{\k@cgs@full@Gravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\k@cgs@full@Gravity| is Newton's gravitational constant in cgs units with % full precision. % Source: CODATA~2018 @@ -5791,24 +12391,250 @@ %<*package> %\fi % \begin{macro}{\kGravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\kGravity| is Newton's gravitational constant. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kGravity}{% -\k@SI@short@Gravity} +\DeclareRobustCommand {\kGravity}{% +\k@SI@short@Gravity} +\else +\DeclareRobustCommand {\kGravity}{% +\k@SI@full@Gravity} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kGravity}{% +\k@cgs@short@Gravity} +\else +\DeclareRobustCommand {\kGravity}{% +\k@cgs@full@Gravity} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@short@GravityNumeric| is Newton's gravitational constant in SI units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@GravityNumeric}{% +\ensuremath{% +6.67e-11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@SI@full@GravityNumeric| is Newton's gravitational constant in SI units with full +% precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@GravityNumeric}{% +\ensuremath{% +6.67430e-11}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@short@GravityNumeric| is Newton's gravitational constant in cgs units with +% reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@GravityNumeric}{% +\ensuremath{% +6.67e-08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@GravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\k@cgs@full@GravityNumeric| is Newton's gravitational constant in cgs units with +% full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@GravityNumeric}{% +\ensuremath{% +6.67430e-08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kGravityNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} +% |\kGravityNumeric| is Newton's gravitational constant. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kGravityNumeric}{% +\k@SI@short@GravityNumeric} +\else +\DeclareRobustCommand {\kGravityNumeric}{% +\k@SI@full@GravityNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kGravityNumeric}{% +\k@cgs@short@GravityNumeric} +\else +\DeclareRobustCommand {\kGravityNumeric}{% +\k@cgs@full@GravityNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@short@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@StefanBoltzmann}{% +\ensuremath{% +5.67% +\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@StefanBoltzmann}{% +\ensuremath{% +5.670\expandafter\physconst@decimalsseparator% +374% +\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@StefanBoltzmann}{% +\ensuremath{% +5.67% +\times 10^{-5}\erg\Kelvin^{-4}\cm^{-2}\Sec^{-1}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@StefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@StefanBoltzmann}{% +\ensuremath{% +5.670\expandafter\physconst@decimalsseparator% +374% +\times 10^{-5}\erg\Kelvin^{-4}\cm^{-2}\Sec^{-1}}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kStefanBoltzmann} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kStefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kStefanBoltzmann}{% +\k@SI@short@StefanBoltzmann} \else -\DeclareRobustCommand {\kGravity}{% -\k@SI@full@Gravity} +\DeclareRobustCommand {\kStefanBoltzmann}{% +\k@SI@full@StefanBoltzmann} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kGravity}{% -\k@cgs@short@Gravity} +\DeclareRobustCommand {\kStefanBoltzmann}{% +\k@cgs@short@StefanBoltzmann} \else -\DeclareRobustCommand {\kGravity}{% -\k@cgs@full@Gravity} +\DeclareRobustCommand {\kStefanBoltzmann}{% +\k@cgs@full@StefanBoltzmann} \fi \fi % \end{macrocode} @@ -5820,17 +12646,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@short@StefanBoltzmann} -% |\k@SI@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% \begin{macro}{\k@SI@short@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@short@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with reduced % precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@short@StefanBoltzmann}{% +\DeclareRobustCommand{\k@SI@short@StefanBoltzmannNumeric}{% \ensuremath{% -5.67% -\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} +5.67e-08}} % \end{macrocode} % \end{macro} % @@ -5840,18 +12666,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@SI@full@StefanBoltzmann} -% |\k@SI@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% \begin{macro}{\k@SI@full@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@SI@full@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in SI units with full % precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@SI@full@StefanBoltzmann}{% +\DeclareRobustCommand{\k@SI@full@StefanBoltzmannNumeric}{% \ensuremath{% -5.670\expandafter\physconst@decimalsseparator% -374% -\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} +5.670374e-08}} % \end{macrocode} % \end{macro} % @@ -5861,17 +12686,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@short@StefanBoltzmann} -% |\k@cgs@short@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% \begin{macro}{\k@cgs@short@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@short@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with reduced % precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@short@StefanBoltzmann}{% +\DeclareRobustCommand{\k@cgs@short@StefanBoltzmannNumeric}{% \ensuremath{% -5.67% -\times 10^{-5}\erg\Kelvin^{-4}\cm^{-2}\Sec^{-1}}} +5.67e-05}} % \end{macrocode} % \end{macro} % @@ -5881,18 +12706,17 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\k@cgs@full@StefanBoltzmann} -% |\k@cgs@full@StefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% \begin{macro}{\k@cgs@full@StefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\k@cgs@full@StefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$ in cgs units with full % precision. % Source: Calculated % % \begin{macrocode} -\DeclareRobustCommand{\k@cgs@full@StefanBoltzmann}{% +\DeclareRobustCommand{\k@cgs@full@StefanBoltzmannNumeric}{% \ensuremath{% -5.670\expandafter\physconst@decimalsseparator% -374% -\times 10^{-5}\erg\Kelvin^{-4}\cm^{-2}\Sec^{-1}}} +5.670374e-05}} % \end{macrocode} % \end{macro} % @@ -5902,26 +12726,27 @@ %\iffalse %<*package> %\fi -% \begin{macro}{\kStefanBoltzmann} -% |\kStefanBoltzmann| is the Stefan-Boltzmann blackbody constant +% \begin{macro}{\kStefanBoltzmannNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} +% |\kStefanBoltzmannNumeric| is the Stefan-Boltzmann blackbody constant % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$. % % \begin{macrocode} \ifx\cgsunits\undefined \ifx\shortconst\undefined -\DeclareRobustCommand {\kStefanBoltzmann}{% -\k@SI@short@StefanBoltzmann} +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@SI@short@StefanBoltzmannNumeric} \else -\DeclareRobustCommand {\kStefanBoltzmann}{% -\k@SI@full@StefanBoltzmann} +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@SI@full@StefanBoltzmannNumeric} \fi \else \ifx\shortconst\undefined -\DeclareRobustCommand {\kStefanBoltzmann}{% -\k@cgs@short@StefanBoltzmann} +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@cgs@short@StefanBoltzmannNumeric} \else -\DeclareRobustCommand {\kStefanBoltzmann}{% -\k@cgs@full@StefanBoltzmann} +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@cgs@full@StefanBoltzmannNumeric} \fi \fi % \end{macrocode} @@ -6046,6 +12871,113 @@ %\iffalse %<*package> %\fi +% \begin{macro}{\k@SI@short@RadiationNumeric} +% |\k@SI@short@RadiationNumeric| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@RadiationNumeric}{% +\ensuremath{% +7.57e-16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@SI@full@RadiationNumeric} +% |\k@SI@full@RadiationNumeric| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in SI units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@full@RadiationNumeric}{% +\ensuremath{% +7.565733e-16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@short@RadiationNumeric} +% |\k@cgs@short@RadiationNumeric| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@short@RadiationNumeric}{% +\ensuremath{% +7.57e-15}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@RadiationNumeric} +% |\k@cgs@full@RadiationNumeric| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$ in cgs units with full +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@RadiationNumeric}{% +\ensuremath{% +7.565733e-15}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiationNumeric} +% |\kRadiationNumeric| is the radiation constant, $a +% \left(\frac{8\pi^5k_\mathrm{B}^4}{15c^3h^3}\right)$. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiationNumeric}{% +\k@SI@short@RadiationNumeric} +\else +\DeclareRobustCommand {\kRadiationNumeric}{% +\k@SI@full@RadiationNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiationNumeric}{% +\k@cgs@short@RadiationNumeric} +\else +\DeclareRobustCommand {\kRadiationNumeric}{% +\k@cgs@full@RadiationNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi % \begin{macro}{\k@short@FineStructure} % |\k@short@FineStructure| is the fine structure constant with reduced % precision. @@ -6105,6 +13037,61 @@ %\iffalse %<*package> %\fi +% \begin{macro}{\k@short@FineStructureNumeric} +% |\k@short@FineStructureNumeric| is the fine structure constant with reduced +% precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@FineStructureNumeric}{% +\ensuremath{% +7.30e-03}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@FineStructureNumeric} +% |\k@full@FineStructureNumeric| is the fine structure constant with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@FineStructureNumeric}{% +\ensuremath{% +7.29735257e-03}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kFineStructureNumeric} +% |\kFineStructureNumeric| is the fine structure constant. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kFineStructureNumeric}{% +\k@short@FineStructureNumeric} +\else +\DeclareRobustCommand {\kFineStructureNumeric}{% +\k@full@FineStructureNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi % \begin{macro}{\k@short@FineStructureReciprocal} % |\k@short@FineStructureReciprocal| is the reciprocal of the fine structure % constant with reduced precision. @@ -6165,6 +13152,62 @@ %\iffalse %<*package> %\fi +% \begin{macro}{\k@short@FineStructureReciprocalNumeric} +% |\k@short@FineStructureReciprocalNumeric| is the reciprocal of the fine structure +% constant with reduced precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@FineStructureReciprocalNumeric}{% +\ensuremath{% +1.37e+02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@FineStructureReciprocalNumeric} +% |\k@full@FineStructureReciprocalNumeric| is the reciprocal of the fine structure +% constant with full precision. +% Source: Calculated +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@FineStructureReciprocalNumeric}{% +\ensuremath{% +1.37035999e+02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kFineStructureReciprocalNumeric} +% |\kFineStructureReciprocalNumeric| is the reciprocal of the fine structure constant. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kFineStructureReciprocalNumeric}{% +\k@short@FineStructureReciprocalNumeric} +\else +\DeclareRobustCommand {\kFineStructureReciprocalNumeric}{% +\k@full@FineStructureReciprocalNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi % \begin{macro}{\k@short@Avogadro} % |\k@short@Avogadro| is Avogadro's Number (the number of particles in a mole) % with reduced precision. @@ -6222,6 +13265,62 @@ %\iffalse % %\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@short@AvogadroNumeric} +% |\k@short@AvogadroNumeric| is Avogadro's Number (the number of particles in a mole) +% with reduced precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@AvogadroNumeric}{% +\ensuremath{% +6.02e+23}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@full@AvogadroNumeric} +% |\k@full@AvogadroNumeric| is Avogadro's Number (the number of particles in a mole) +% with full precision. +% Source: CODATA~2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@full@AvogadroNumeric}{% +\ensuremath{% +6.02240760e+23}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kAvogadroNumeric} +% |\kAvogadroNumeric| is Avogadro's Number (the number of particles in a mole). +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kAvogadroNumeric}{% +\k@short@AvogadroNumeric} +\else +\DeclareRobustCommand {\kAvogadroNumeric}{% +\k@full@AvogadroNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +% +%\fi % \CheckSum{0} % \Finale \makeatother diff --git a/macros/latex/contrib/physconst/physconst.pdf b/macros/latex/contrib/physconst/physconst.pdf index 67867850bc..ead2ea8bc7 100644 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