diff options
author | Karl Berry <karl@freefriends.org> | 2020-02-04 22:19:29 +0000 |
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committer | Karl Berry <karl@freefriends.org> | 2020-02-04 22:19:29 +0000 |
commit | 16a594a6cdc908144e115e563592fdf21a3fb950 (patch) | |
tree | 075d34384b3ca12638314ffd11b5cf1125ac92a6 /Master/texmf-dist/source | |
parent | c4f9025af51074274f379c8470324c4e7839780a (diff) |
physconst (4feb20)
git-svn-id: svn://tug.org/texlive/trunk@53674 c570f23f-e606-0410-a88d-b1316a301751
Diffstat (limited to 'Master/texmf-dist/source')
-rw-r--r-- | Master/texmf-dist/source/latex/physconst/physconst.dtx | 7281 |
1 files changed, 7190 insertions, 91 deletions
diff --git a/Master/texmf-dist/source/latex/physconst/physconst.dtx b/Master/texmf-dist/source/latex/physconst/physconst.dtx index 691a5fd9018..7ade1893813 100644 --- a/Master/texmf-dist/source/latex/physconst/physconst.dtx +++ b/Master/texmf-dist/source/latex/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) @@ -461,7 +763,121 @@ % {The value is \k@eV@full@MassElectron}\end{mdframed} % \makeatother % +% \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@MassElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@MassElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@MassElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@MassElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@MassElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@MassElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@MassElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@MassElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@MassElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@MassElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@MassElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@MassElectronNumeric}\end{mdframed} +% \makeatother +% % \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) @@ -478,6 +894,8 @@ % \makeatother % % \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) @@ -494,6 +912,8 @@ % \makeatother % % \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) @@ -510,6 +930,8 @@ % \makeatother % % \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) @@ -526,6 +948,8 @@ % \makeatother % % \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) % @@ -541,6 +965,8 @@ % \makeatother % % \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) % @@ -555,7 +981,119 @@ % {The value is \k@eV@full@MassProton}\end{mdframed} % \makeatother % +% \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. +% (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@MassProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@MassProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@MassProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@MassProtonNumeric}\end{mdframed} +% \makeatother +% +% \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. +% (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@MassProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@MassProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@MassProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@MassProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@eV@short@MassProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@MassProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@eV@full@MassProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@MassProtonNumeric}\end{mdframed} +% \makeatother +% % \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) @@ -572,6 +1110,8 @@ % \makeatother % % \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) @@ -588,6 +1128,8 @@ % \makeatother % % \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) @@ -604,6 +1146,8 @@ % \makeatother % % \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) @@ -620,6 +1164,8 @@ % \makeatother % % \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) @@ -636,6 +1182,8 @@ % \makeatother % % \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) @@ -651,6 +1199,120 @@ % {The value is \k@eV@full@MassHydrogen}\end{mdframed} % \makeatother % +% \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@SI@short@MassHydrogenNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@MassHydrogenNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@MassHydrogenNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@MassHydrogenNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@MassHydrogenNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@MassHydrogenNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@MassHydrogenNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@MassHydrogenNumeric}\end{mdframed} +% \makeatother +% +% \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@eV@short@MassHydrogenNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@MassHydrogenNumeric}\end{mdframed} +% \makeatother +% +% \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@eV@full@MassHydrogenNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@MassHydrogenNumeric}\end{mdframed} +% \makeatother +% % \DescribeMacro{\k@SI@short@MassSun} % |\k@SI@short@MassSun| is the mass of the Sun in SI units with reduced % precision. @@ -713,7 +1375,205 @@ % {The value is \k@cgs@full@MassSun}\end{mdframed} % \makeatother % +% \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@MassSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@MassSunNumeric}\end{mdframed} +% \makeatother +% +% \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@MassSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@MassSunNumeric}\end{mdframed} +% \makeatother +% +% \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@MassSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@MassSunNumeric}\end{mdframed} +% \makeatother +% +% \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@MassSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@MassSunNumeric}\end{mdframed} +% \makeatother +% +% \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@short@MassEarth\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@MassEarth}\end{mdframed} +% \makeatother +% +% \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@full@MassEarth\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@MassEarth}\end{mdframed} +% \makeatother +% +% \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@short@MassEarthNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@MassEarthNumeric}\end{mdframed} +% \makeatother +% +% \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@full@MassEarthNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@MassEarthNumeric}\end{mdframed} +% \makeatother +% +% \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@short@MassJupiter\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@MassJupiter}\end{mdframed} +% \makeatother +% +% \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@full@MassJupiter\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@MassJupiter}\end{mdframed} +% \makeatother +% +% \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@short@MassJupiterNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@short@MassJupiterNumeric}\end{mdframed} +% \makeatother +% +% \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@full@MassJupiterNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@full@MassJupiterNumeric}\end{mdframed} +% \makeatother +% % \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. % (CODATA~2018) @@ -730,6 +1590,8 @@ % \makeatother % % \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. % (CODATA~2018) @@ -746,6 +1608,8 @@ % \makeatother % % \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. % (CODATA~2018) @@ -762,6 +1626,8 @@ % \makeatother % % \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) @@ -778,6 +1644,8 @@ % \makeatother % % \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) @@ -794,6 +1662,8 @@ % \makeatother % % \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) @@ -809,6 +1679,119 @@ % {The value is \k@eV@full@MassAMU}\end{mdframed} % \makeatother % +% \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@SI@short@MassAMUNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@MassAMUNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@MassAMUNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@MassAMUNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@MassAMUNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@MassAMUNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@MassAMUNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@MassAMUNumeric}\end{mdframed} +% \makeatother +% +% \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@eV@short@MassAMUNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@MassAMUNumeric}\end{mdframed} +% \makeatother +% +% \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@eV@full@MassAMUNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@MassAMUNumeric}\end{mdframed} +% \makeatother +% % %\subsubsection{Charge} % @@ -876,6 +1859,74 @@ % {The value is \k@cgs@full@ChargeFundamental}\end{mdframed} % \makeatother % +% \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@SI@short@ChargeFundamentalNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@ChargeFundamentalNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@ChargeFundamentalNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@ChargeFundamentalNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@ChargeFundamentalNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@ChargeFundamentalNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@ChargeFundamentalNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@ChargeFundamentalNumeric}\end{mdframed} +% \makeatother +% % \DescribeMacro{\k@SI@short@ChargeElectron} % |\k@SI@short@ChargeElectron| is the charge of an electron in SI units with % reduced precision. @@ -940,6 +1991,74 @@ % {The value is \k@cgs@full@ChargeElectron}\end{mdframed} % \makeatother % +% \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) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@short@ChargeElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@ChargeElectronNumeric}\end{mdframed} +% \makeatother +% +% \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) +% +% The macro can be invoked by (e.g.) +% \begin{mdframed}[backgroundcolor=orange!25]% +% {\small\texttt{\textbackslash makeatletter\\ The value is +% \textbackslash k@SI@full@ChargeElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@ChargeElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@ChargeElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@ChargeElectronNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@ChargeElectronNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@ChargeElectronNumeric}\end{mdframed} +% \makeatother +% % \DescribeMacro{\k@SI@short@ChargeProton} % |\k@SI@short@ChargeProton| is the charge of a proton in SI units with reduced % precision. @@ -1004,6 +2123,74 @@ % {The value is \k@cgs@full@ChargeProton}\end{mdframed} % \makeatother % +% \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@SI@short@ChargeProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@ChargeProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@ChargeProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@ChargeProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@ChargeProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@ChargeProtonNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@ChargeProtonNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@ChargeProtonNumeric}\end{mdframed} +% \makeatother +% % %\subsubsection{Distances and Lengths} % @@ -1071,6 +2258,73 @@ % {The value is \k@cgs@full@RadiusBohr}\end{mdframed} % \makeatother % +% \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@SI@short@RadiusBohrNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@RadiusBohrNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@RadiusBohrNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@RadiusBohrNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@RadiusBohrNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@RadiusBohrNumeric}\end{mdframed} +% \makeatother +% +% \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. +% (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@RadiusBohrNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@RadiusBohrNumeric}\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. @@ -1135,6 +2389,74 @@ % {The value is \k@cgs@full@AstronomicalUnit}\end{mdframed} % \makeatother % +% \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@SI@short@AstronomicalUnitNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@AstronomicalUnitNumeric}\end{mdframed} +% \makeatother +% +% \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@full@AstronomicalUnitNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@AstronomicalUnitNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@AstronomicalUnitNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@AstronomicalUnitNumeric}\end{mdframed} +% \makeatother +% +% \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@full@AstronomicalUnitNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@AstronomicalUnitNumeric}\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. @@ -1199,6 +2521,74 @@ % {The value is \k@cgs@full@Parsec}\end{mdframed} % \makeatother % +% \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@short@ParsecNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@ParsecNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@ParsecNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@ParsecNumeric}\end{mdframed} +% \makeatother +% +% \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@short@ParsecNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@ParsecNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@ParsecNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@ParsecNumeric}\end{mdframed} +% \makeatother +% % \DescribeMacro{\k@SI@short@RadiusSun} % |\k@SI@short@RadiusSun| is the mean radius of the Sun in SI units with % reduced precision. @@ -1263,6 +2653,206 @@ % {The value is \k@cgs@full@RadiusSun}\end{mdframed} % \makeatother % +% \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@SI@short@RadiusSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@RadiusSunNumeric}\end{mdframed} +% \makeatother +% +% \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. +% (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@RadiusSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@RadiusSunNumeric}\end{mdframed} +% \makeatother +% +% \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. +% (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@RadiusSunNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@RadiusSunNumeric}\end{mdframed} +% \makeatother +% +% \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} % @@ -1362,6 +2952,108 @@ % {The value is \k@eV@full@Rydberg}\end{mdframed} % \makeatother % +% \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@SI@short@RydbergNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@short@RydbergNumeric}\end{mdframed} +% \makeatother +% +% \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@SI@full@RydbergNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@SI@full@RydbergNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@short@RydbergNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@short@RydbergNumeric}\end{mdframed} +% \makeatother +% +% \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@cgs@full@RydbergNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@cgs@full@RydbergNumeric}\end{mdframed} +% \makeatother +% +% \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. +% (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@RydbergNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@short@RydbergNumeric}\end{mdframed} +% \makeatother +% +% \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. +% (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@RydbergNumeric\\ +% \textbackslash makeatother}}\end{mdframed} +% \makeatletter +% Resulting in +% \begin{mdframed}[backgroundcolor=blue!25]% +% {The value is \k@eV@full@RydbergNumeric}\end{mdframed} +% \makeatother +% % \DescribeMacro{\k@SI@short@LuminositySun} % |\k@SI@short@LuminositySun| is the luminosity of the Sun in SI units with % reduced precision. @@ -1426,10 +3118,79 @@ % {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) @@ -1446,6 +3207,7 @@ % \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) @@ -1462,6 +3224,7 @@ % \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) @@ -1478,6 +3241,7 @@ % \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) @@ -1493,7 +3257,80 @@ % {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) @@ -1510,6 +3347,7 @@ % \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) @@ -1526,6 +3364,7 @@ % \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) @@ -1542,6 +3381,7 @@ % \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) @@ -1557,6 +3397,78 @@ % {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} % @@ -1623,7 +3535,74 @@ % {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) @@ -1640,6 +3619,8 @@ % \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) @@ -1656,6 +3637,8 @@ % \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) @@ -1672,6 +3655,8 @@ % \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) @@ -1687,10 +3672,87 @@ % {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) @@ -1707,6 +3769,7 @@ % \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) @@ -1723,6 +3786,7 @@ % \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) @@ -1739,6 +3803,7 @@ % \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) @@ -1754,6 +3819,78 @@ % {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. @@ -1818,10 +3955,79 @@ % {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. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% @@ -1835,9 +4041,10 @@ % \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. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% @@ -1851,9 +4058,10 @@ % \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. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% @@ -1867,9 +4075,10 @@ % \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. -% (CODATA~2018) +% (Calculated) % % The macro can be invoked by (e.g.) % \begin{mdframed}[backgroundcolor=orange!25]% @@ -1882,6 +4091,78 @@ % {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. @@ -1914,6 +4195,40 @@ % {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. @@ -2009,7 +4324,106 @@ % {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) @@ -2026,6 +4440,7 @@ % \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) % @@ -2041,6 +4456,7 @@ % \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) @@ -2057,6 +4473,7 @@ % \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) % @@ -2072,6 +4489,7 @@ % \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) % @@ -2087,6 +4505,7 @@ % \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) % @@ -2101,7 +4520,110 @@ % {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) @@ -2118,6 +4640,7 @@ % \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) @@ -2134,6 +4657,7 @@ % \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) @@ -2150,6 +4674,7 @@ % \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) @@ -2166,6 +4691,7 @@ % \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) @@ -2182,6 +4708,7 @@ % \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) @@ -2197,7 +4724,116 @@ % {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) @@ -2214,6 +4850,7 @@ % \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) @@ -2230,6 +4867,7 @@ % \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) @@ -2246,6 +4884,7 @@ % \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) @@ -2261,7 +4900,80 @@ % {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. @@ -2279,6 +4991,7 @@ % \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. @@ -2296,6 +5009,7 @@ % \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. @@ -2313,6 +5027,7 @@ % \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. @@ -2329,6 +5044,82 @@ % {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 @@ -2397,6 +5188,78 @@ % {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. @@ -2428,6 +5291,38 @@ % {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. @@ -2460,6 +5355,40 @@ % {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. @@ -2492,6 +5421,40 @@ % {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{} % @@ -2527,6 +5490,8 @@ %<*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 @@ -2535,7 +5500,7 @@ \DeclareRobustCommand{\k@SI@short@MassElectron}{% \ensuremath{% 9.11% -\times 10^{-34}\kg}} +\times 10^{-31}\kg}} % \end{macrocode} % \end{macro} % @@ -2546,6 +5511,8 @@ %<*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 @@ -2557,7 +5524,7 @@ 980\expandafter\physconst@decimalsseparator% 087\expandafter\physconst@decimalsseparator% 382% -\times 10^{-34}\kg}} +\times 10^{-31}\kg}} % \end{macrocode} % \end{macro} % @@ -2568,6 +5535,8 @@ %<*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 @@ -2576,7 +5545,7 @@ \DeclareRobustCommand{\k@cgs@short@MassElectron}{% \ensuremath{% 9.11% -\times 10^{-31}\gm}} +\times 10^{-28}\gm}} % \end{macrocode} % \end{macro} % @@ -2587,6 +5556,8 @@ %<*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 @@ -2598,7 +5569,7 @@ 980\expandafter\physconst@decimalsseparator% 087\expandafter\physconst@decimalsseparator% 382% -\times 10^{-31}\gm}} +\times 10^{-28}\gm}} % \end{macrocode} % \end{macro} % @@ -2609,6 +5580,8 @@ %<*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 @@ -2616,8 +5589,8 @@ % \begin{macrocode} \DeclareRobustCommand{\k@eV@short@MassElectron}{% \ensuremath{% -5.69% -\times 10^{-19}\eV\,c^{-2}}} +5.11% +\times 10^{5}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -2628,6 +5601,8 @@ %<*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 @@ -2635,11 +5610,11 @@ % \begin{macrocode} \DeclareRobustCommand{\k@eV@full@MassElectron}{% \ensuremath{% -5.685\expandafter\physconst@decimalsseparator% -378\expandafter\physconst@decimalsseparator% -187\expandafter\physconst@decimalsseparator% -448% -\times 10^{-19}\eV\,c^{-2}}} +5.109\expandafter\physconst@decimalsseparator% +763\expandafter\physconst@decimalsseparator% +089\expandafter\physconst@decimalsseparator% +046% +\times 10^{5}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -2650,6 +5625,8 @@ %<*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} @@ -2680,6 +5657,8 @@ %<*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} @@ -2699,7 +5678,183 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 @@ -2708,7 +5863,7 @@ \DeclareRobustCommand{\k@SI@short@MassProton}{% \ensuremath{% 1.67% -\times 10^{-30}\kg}} +\times 10^{-27}\kg}} % \end{macrocode} % \end{macro} % @@ -2719,6 +5874,8 @@ %<*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 @@ -2730,7 +5887,7 @@ 547\expandafter\physconst@decimalsseparator% 813\expandafter\physconst@decimalsseparator% 969% -\times 10^{-30}\kg}} +\times 10^{-27}\kg}} % \end{macrocode} % \end{macro} % @@ -2741,6 +5898,8 @@ %<*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 @@ -2749,7 +5908,7 @@ \DeclareRobustCommand{\k@cgs@short@MassProton}{% \ensuremath{% 1.67% -\times 10^{-27}\gm}} +\times 10^{-24}\gm}} % \end{macrocode} % \end{macro} % @@ -2760,6 +5919,8 @@ %<*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 @@ -2771,7 +5932,7 @@ 547\expandafter\physconst@decimalsseparator% 813\expandafter\physconst@decimalsseparator% 969% -\times 10^{-27}\gm}} +\times 10^{-24}\gm}} % \end{macrocode} % \end{macro} % @@ -2782,14 +5943,16 @@ %<*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{% -1.04% -\times 10^{-15}\eV\,c^{-2}}} +9.38% +\times 10^{8}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -2800,17 +5963,19 @@ %<*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{% -1.043\expandafter\physconst@decimalsseparator% -922\expandafter\physconst@decimalsseparator% -235\expandafter\physconst@decimalsseparator% -836% -\times 10^{-15}\eV\,c^{-2}}} +9.382\expandafter\physconst@decimalsseparator% +305\expandafter\physconst@decimalsseparator% +156\expandafter\physconst@decimalsseparator% +558% +\times 10^{8}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -2821,6 +5986,8 @@ %<*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} @@ -2851,6 +6018,8 @@ %<*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} @@ -2870,7 +6039,181 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 @@ -2879,7 +6222,7 @@ \DeclareRobustCommand{\k@SI@short@MassHydrogen}{% \ensuremath{% 1.67% -\times 10^{-30}\kg}} +\times 10^{-27}\kg}} % \end{macrocode} % \end{macro} % @@ -2890,6 +6233,8 @@ %<*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 @@ -2901,7 +6246,7 @@ 458\expandafter\physconst@decimalsseparator% 687\expandafter\physconst@decimalsseparator% 724% -\times 10^{-30}\kg}} +\times 10^{-27}\kg}} % \end{macrocode} % \end{macro} % @@ -2912,6 +6257,8 @@ %<*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 @@ -2920,7 +6267,7 @@ \DeclareRobustCommand{\k@cgs@short@MassHydrogen}{% \ensuremath{% 1.67% -\times 10^{-27}\gm}} +\times 10^{-24}\gm}} % \end{macrocode} % \end{macro} % @@ -2931,6 +6278,8 @@ %<*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 @@ -2942,7 +6291,7 @@ 458\expandafter\physconst@decimalsseparator% 687\expandafter\physconst@decimalsseparator% 724% -\times 10^{-27}\gm}} +\times 10^{-24}\gm}} % \end{macrocode} % \end{macro} % @@ -2953,6 +6302,8 @@ %<*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 @@ -2960,8 +6311,8 @@ % \begin{macrocode} \DeclareRobustCommand{\k@eV@short@MassHydrogen}{% \ensuremath{% -1.04% -\times 10^{-15}\eV\,c^{-2}}} +9.39% +\times 10^{8}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -2972,6 +6323,8 @@ %<*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 @@ -2979,11 +6332,11 @@ % \begin{macrocode} \DeclareRobustCommand{\k@eV@full@MassHydrogen}{% \ensuremath{% -1.044\expandafter\physconst@decimalsseparator% -490\expandafter\physconst@decimalsseparator% -758\expandafter\physconst@decimalsseparator% -517% -\times 10^{-15}\eV\,c^{-2}}} +9.387\expandafter\physconst@decimalsseparator% +414\expandafter\physconst@decimalsseparator% +783\expandafter\physconst@decimalsseparator% +596% +\times 10^{8}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -2994,6 +6347,8 @@ %<*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} @@ -3024,6 +6379,8 @@ %<*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} @@ -3043,6 +6400,180 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -3151,7 +6682,344 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 @@ -3160,7 +7028,7 @@ \DeclareRobustCommand{\k@SI@short@MassAMU}{% \ensuremath{% 1.66% -\times 10^{-30}\kg}} +\times 10^{-27}\kg}} % \end{macrocode} % \end{macro} % @@ -3171,6 +7039,8 @@ %<*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 @@ -3182,7 +7052,7 @@ 465\expandafter\physconst@decimalsseparator% 492\expandafter\physconst@decimalsseparator% 239% -\times 10^{-30}\kg}} +\times 10^{-27}\kg}} % \end{macrocode} % \end{macro} % @@ -3193,6 +7063,8 @@ %<*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 @@ -3201,7 +7073,7 @@ \DeclareRobustCommand{\k@cgs@short@MassAMU}{% \ensuremath{% 1.66% -\times 10^{-27}\gm}} +\times 10^{-24}\gm}} % \end{macrocode} % \end{macro} % @@ -3212,6 +7084,8 @@ %<*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 @@ -3223,7 +7097,7 @@ 465\expandafter\physconst@decimalsseparator% 492\expandafter\physconst@decimalsseparator% 239% -\times 10^{-27}\gm}} +\times 10^{-24}\gm}} % \end{macrocode} % \end{macro} % @@ -3234,6 +7108,8 @@ %<*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 @@ -3241,8 +7117,8 @@ % \begin{macrocode} \DeclareRobustCommand{\k@eV@short@MassAMU}{% \ensuremath{% -1.04% -\times 10^{-15}\eV\,c^{-2}}} +9.31% +\times 10^{8}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -3253,6 +7129,8 @@ %<*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 @@ -3260,11 +7138,11 @@ % \begin{macrocode} \DeclareRobustCommand{\k@eV@full@MassAMU}{% \ensuremath{% -1.036\expandafter\physconst@decimalsseparator% -381\expandafter\physconst@decimalsseparator% -043\expandafter\physconst@decimalsseparator% -764% -\times 10^{-15}\eV\,c^{-2}}} +9.314\expandafter\physconst@decimalsseparator% +528\expandafter\physconst@decimalsseparator% +302\expandafter\physconst@decimalsseparator% +276% +\times 10^{8}\eV\,c^{-2}}} % \end{macrocode} % \end{macro} % @@ -3275,6 +7153,8 @@ %<*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} @@ -3305,6 +7185,8 @@ %<*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} @@ -3321,6 +7203,180 @@ %\iffalse %</package> %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\fi % %\subsection{Charge} % @@ -3437,6 +7493,108 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -3547,6 +7705,108 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -3654,6 +7914,108 @@ %\iffalse %</package> %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\fi % %\subsection{Distances and Lengths} % @@ -3669,7 +8031,7 @@ \DeclareRobustCommand{\k@SI@short@RadiusBohr}{% \ensuremath{% 5.29% -\times 10^{-8}\m}} +\times 10^{-11}\m}} % \end{macrocode} % \end{macro} % @@ -3690,7 +8052,7 @@ 5.292\expandafter\physconst@decimalsseparator% 006\expandafter\physconst@decimalsseparator% 59% -\times 10^{-8}\m}} +\times 10^{-11}\m}} % \end{macrocode} % \end{macro} % @@ -3709,7 +8071,7 @@ \DeclareRobustCommand{\k@cgs@short@RadiusBohr}{% \ensuremath{% 5.29% -\times 10^{-6}\cm}} +\times 10^{-9}\cm}} % \end{macrocode} % \end{macro} % @@ -3730,7 +8092,7 @@ 5.292\expandafter\physconst@decimalsseparator% 006\expandafter\physconst@decimalsseparator% 59% -\times 10^{-6}\cm}} +\times 10^{-9}\cm}} % \end{macrocode} % \end{macro} % @@ -3770,6 +8132,108 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -3881,6 +8345,109 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -3991,6 +8558,108 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -4094,6 +8763,342 @@ %\iffalse %</package> %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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} +\DeclareRobustCommand{\k@full@RadiusJupiter}{% +\ensuremath{% +6.991\expandafter\physconst@decimalsseparator% +1% +\times 10^{7}\m}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\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 {\kRadiusJupiter}{% +\k@full@RadiusJupiter} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\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 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@short@RadiusJupiterNumeric}{% +\ensuremath{% +6.99e+07}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@full@RadiusJupiterNumeric}{% +\ensuremath{% +6.9911e+07}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRadiusJupiterNumeric} +% \changes{v1.1.0}{2020/02/03}{Add radius of Jupiter} +% |\kRadiusJupiterNumeric| is the mean radius of Jupiter. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kRadiusJupiterNumeric}{% +\k@short@RadiusJupiterNumeric} +\else +\DeclareRobustCommand {\kRadiusJupiterNumeric}{% +\k@full@RadiusJupiterNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi % %\subsection{Energy, Power, and Luminosity} % @@ -4109,7 +9114,7 @@ \DeclareRobustCommand{\k@SI@short@Rydberg}{% \ensuremath{% 2.18% -\times 10^{-21}\Joule}} +\times 10^{-18}\Joule}} % \end{macrocode} % \end{macro} % @@ -4130,7 +9135,7 @@ 2.179\expandafter\physconst@decimalsseparator% 775\expandafter\physconst@decimalsseparator% 77% -\times 10^{-21}\Joule}} +\times 10^{-18}\Joule}} % \end{macrocode} % \end{macro} % @@ -4149,7 +9154,7 @@ \DeclareRobustCommand{\k@cgs@short@Rydberg}{% \ensuremath{% 2.18% -\times 10^{-14}\erg}} +\times 10^{-11}\erg}} % \end{macrocode} % \end{macro} % @@ -4170,7 +9175,7 @@ 2.179\expandafter\physconst@decimalsseparator% 775\expandafter\physconst@decimalsseparator% 77% -\times 10^{-14}\erg}} +\times 10^{-11}\erg}} % \end{macrocode} % \end{macro} % @@ -4189,7 +9194,7 @@ \DeclareRobustCommand{\k@eV@short@Rydberg}{% \ensuremath{% 1.36% -\times 10^{-2}\eV}} +\times 10^{1}\eV}} % \end{macrocode} % \end{macro} % @@ -4210,7 +9215,7 @@ 1.360\expandafter\physconst@decimalsseparator% 509\expandafter\physconst@decimalsseparator% 03% -\times 10^{-2}\eV}} +\times 10^{1}\eV}} % \end{macrocode} % \end{macro} % @@ -4270,6 +9275,164 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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} +\DeclareRobustCommand{\k@eV@short@RydbergNumeric}{% +\ensuremath{% +1.36e+01}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@eV@full@RydbergNumeric}{% +\ensuremath{% +1.36050903e+01}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kRydbergNumeric} +% |\kRydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen). +% +% \begin{macrocode} +\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} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVRydbergNumeric} +% |\keVRydbergNumeric| is the Rydberg energy (the binding energy of Hydrogen). +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVRydbergNumeric}{% +\k@eV@short@RydbergNumeric} +\else +\DeclareRobustCommand {\keVRydbergNumeric}{% +\k@eV@full@RydbergNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\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. @@ -4373,6 +9536,108 @@ %\iffalse %</package> %\fi +%\iffalse +%<*package> +%\fi +% \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@LuminositySunNumeric}{% +\ensuremath{% +3.83e+26}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@LuminositySunNumeric}{% +\ensuremath{% +3.828e+26}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@LuminositySunNumeric}{% +\ensuremath{% +3.83e+33}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@LuminositySunNumeric}{% +\ensuremath{% +3.828e+33}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kLuminositySunNumeric} +% |\kLuminositySunNumeric| is the luminosity of the Sun. +% +% \begin{macrocode} +\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 +%</package> +%\fi % %\subsection{Pressure} % @@ -4380,6 +9645,7 @@ %<*package> %\fi % \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 @@ -4399,6 +9665,7 @@ %<*package> %\fi % \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 @@ -4419,6 +9686,7 @@ %<*package> %\fi % \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 @@ -4426,7 +9694,7 @@ % \begin{macrocode} \DeclareRobustCommand{\k@cgs@short@PressureAtmosphere}{% \ensuremath{% -1.01\barP[m]}} +1.01\barP}} % \end{macrocode} % \end{macro} % @@ -4437,6 +9705,7 @@ %<*package> %\fi % \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 @@ -4445,7 +9714,7 @@ \DeclareRobustCommand{\k@cgs@full@PressureAtmosphere}{% \ensuremath{% 1.013\expandafter\physconst@decimalsseparator% -25\barP[m]}} +25\barP}} % \end{macrocode} % \end{macro} % @@ -4456,6 +9725,7 @@ %<*package> %\fi % \begin{macro}{\kPressureAtmosphere} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} % |\kPressureAtmosphere| is the standard atmospheric pressure. % % \begin{macrocode} @@ -4485,7 +9755,115 @@ %\iffalse %<*package> %\fi +% \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@SI@short@PressureAtmosphereNumeric}{% +\ensuremath{% +1.01e+05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@SI@full@PressureAtmosphereNumeric}{% +\ensuremath{% +1.01325e+05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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} +\DeclareRobustCommand{\k@cgs@short@PressureAtmosphereNumeric}{% +\ensuremath{% +1.01e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@cgs@full@PressureAtmosphereNumeric}{% +\ensuremath{% +1.01325e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kPressureAtmosphereNumeric} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} +% |\kPressureAtmosphereNumeric| is the standard atmospheric pressure. +% +% \begin{macrocode} +\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} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \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 @@ -4505,6 +9883,7 @@ %<*package> %\fi % \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 @@ -4525,6 +9904,7 @@ %<*package> %\fi % \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 @@ -4532,7 +9912,7 @@ % \begin{macrocode} \DeclareRobustCommand{\k@cgs@short@PressureStandard}{% \ensuremath{% -1.00\barP[m]}} +1.00\barP}} % \end{macrocode} % \end{macro} % @@ -4543,6 +9923,7 @@ %<*package> %\fi % \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 @@ -4551,7 +9932,7 @@ \DeclareRobustCommand{\k@cgs@full@PressureStandard}{% \ensuremath{% 1.000\expandafter\physconst@decimalsseparator% -00\barP[m]}} +00\barP}} % \end{macrocode} % \end{macro} % @@ -4562,6 +9943,7 @@ %<*package> %\fi % \begin{macro}{\kPressureStandard} +% \changes{v1.1.0}{2020/02/03}{Fix prefix of units.} % |\kPressureStandard| is the standard atmospheric pressure. % % \begin{macrocode} @@ -4588,6 +9970,113 @@ %\iffalse %</package> %\fi +%\iffalse +%<*package> +%\fi +% \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@PressureStandardNumeric}{% +\ensuremath{% +1.00e+05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PressureStandardNumeric}{% +\ensuremath{% +1.00000e+05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PressureStandardNumeric}{% +\ensuremath{% +1.00e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PressureStandardNumeric}{% +\ensuremath{% +1.00000e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kPressureStandardNumeric}{% +\k@SI@short@PressureStandardNumeric} +\else +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@SI@full@PressureStandardNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@cgs@short@PressureStandardNumeric} +\else +\DeclareRobustCommand {\kPressureStandardNumeric}{% +\k@cgs@full@PressureStandardNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi % %\subsection{Velocity, Speed and Acceleration} % @@ -4703,7 +10192,110 @@ %\iffalse %<*package> %\fi +% \begin{macro}{\k@SI@short@SpeedLightNumeric} +% |\k@SI@short@SpeedLightNumeric| is the speed of light in SI units with reduced +% precision. +% Source: CODATA 2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@SI@short@SpeedLightNumeric}{% +\ensuremath{% +3.00e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@SpeedLightNumeric}{% +\ensuremath{% +2.99792458e+08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@SpeedLightNumeric}{% +\ensuremath{% +3.00e+10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\k@cgs@full@SpeedLightNumeric} +% |\k@cgs@full@SpeedLightNumeric| is the speed of light in cgs units with full +% precision. +% Source: CODATA 2018 +% +% \begin{macrocode} +\DeclareRobustCommand{\k@cgs@full@SpeedLightNumeric}{% +\ensuremath{% +2.99792458e+10}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kSpeedLightNumeric} +% |\kSpeedLightNumeric| is the speed of light. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@SI@short@SpeedLightNumeric} +\else +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@SI@full@SpeedLightNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@cgs@short@SpeedLightNumeric} +\else +\DeclareRobustCommand {\kSpeedLightNumeric}{% +\k@cgs@full@SpeedLightNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \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 @@ -4711,8 +10303,7 @@ % \begin{macrocode} \DeclareRobustCommand{\k@SI@short@AccelGravity}{% \ensuremath{% -6.67% -\times 10^{-11}\N\kg^{-2}\m^2}} +9.81\m\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -4723,6 +10314,8 @@ %<*package> %\fi % \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 @@ -4730,9 +10323,8 @@ % \begin{macrocode} \DeclareRobustCommand{\k@SI@full@AccelGravity}{% \ensuremath{% -6.674\expandafter\physconst@decimalsseparator% -30% -\times 10^{-11}\N\kg^{-2}\m^2}} +9.806\expandafter\physconst@decimalsseparator% +65\m\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -4743,6 +10335,8 @@ %<*package> %\fi % \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 @@ -4750,8 +10344,8 @@ % \begin{macrocode} \DeclareRobustCommand{\k@cgs@short@AccelGravity}{% \ensuremath{% -6.67% -\times 10^{-8}\dyne\gm^{-2}\cm^2}} +9.81% +\times 10^{2}\cm\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -4762,6 +10356,8 @@ %<*package> %\fi % \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 @@ -4769,9 +10365,9 @@ % \begin{macrocode} \DeclareRobustCommand{\k@cgs@full@AccelGravity}{% \ensuremath{% -6.674\expandafter\physconst@decimalsseparator% -30% -\times 10^{-8}\dyne\gm^{-2}\cm^2}} +9.806\expandafter\physconst@decimalsseparator% +65% +\times 10^{2}\cm\Sec^{-2}}} % \end{macrocode} % \end{macro} % @@ -4782,6 +10378,8 @@ %<*package> %\fi % \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. % @@ -4809,6 +10407,119 @@ %\iffalse %</package> %\fi +%\iffalse +%<*package> +%\fi +% \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@AccelGravityNumeric}{% +\ensuremath{% +9.81e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@AccelGravityNumeric}{% +\ensuremath{% +9.80665e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@AccelGravityNumeric}{% +\ensuremath{% +9.81e+02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@AccelGravityNumeric}{% +\ensuremath{% +9.80665e+02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kAccelGravityNumeric}{% +\k@SI@short@AccelGravityNumeric} +\else +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@SI@full@AccelGravityNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@cgs@short@AccelGravityNumeric} +\else +\DeclareRobustCommand {\kAccelGravityNumeric}{% +\k@cgs@full@AccelGravityNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi % %\subsection{Other Constants} % @@ -4816,6 +10527,7 @@ %<*package> %\fi % \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 @@ -4824,7 +10536,7 @@ \DeclareRobustCommand{\k@SI@short@Coulomb}{% \ensuremath{% 8.99% -\times 10^{13}\N\m^2\Coulomb^{-2}}} +\times 10^{9}\N\m^2\Coulomb^{-2}}} % \end{macrocode} % \end{macro} % @@ -4835,6 +10547,7 @@ %<*package> %\fi % \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 @@ -4845,7 +10558,7 @@ 8.987\expandafter\physconst@decimalsseparator% 551\expandafter\physconst@decimalsseparator% 79% -\times 10^{13}\N\m^2\Coulomb^{-2}}} +\times 10^{9}\N\m^2\Coulomb^{-2}}} % \end{macrocode} % \end{macro} % @@ -4856,6 +10569,7 @@ %<*package> %\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 @@ -4874,6 +10588,7 @@ %<*package> %\fi % \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 @@ -4894,6 +10609,7 @@ %<*package> %\fi % \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} @@ -4923,6 +10639,113 @@ %\iffalse %<*package> %\fi +% \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@CoulombNumeric}{% +\ensuremath{% +8.99e+09}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@CoulombNumeric}{% +\ensuremath{% +8.98755179e+09}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@CoulombNumeric}{% +\ensuremath{% +1.00e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@CoulombNumeric}{% +\ensuremath{% +1.00000000e+00}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kCoulombNumeric}{% +\k@SI@short@CoulombNumeric} +\else +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@SI@full@CoulombNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@cgs@short@CoulombNumeric} +\else +\DeclareRobustCommand {\kCoulombNumeric}{% +\k@cgs@full@CoulombNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\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. @@ -5035,16 +10858,119 @@ %\iffalse %<*package> %\fi +% \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@VacuumPermittivityNumeric}{% +\ensuremath{% +8.85e-12}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@VacuumPermittivityNumeric}{% +\ensuremath{% +8.8541878128e-12}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@VacuumPermittivityNumeric}{% +\ensuremath{% +7.96e-02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@VacuumPermittivityNumeric}{% +\ensuremath{% +7.9577471546e-02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kVacuumPermittivityNumeric} +% |\kVacuumPermittivityNumeric| is the electric permittivity of the vacuum. +% +% \begin{macrocode} +\ifx\cgsunits\undefined +\ifx\shortconst\undefined +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@SI@short@VacuumPermittivityNumeric} +\else +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@SI@full@VacuumPermittivityNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@cgs@short@VacuumPermittivityNumeric} +\else +\DeclareRobustCommand {\kVacuumPermittivityNumeric}{% +\k@cgs@full@VacuumPermittivityNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \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: CODATA~2018 +% Source: Calculated % % \begin{macrocode} \DeclareRobustCommand{\k@SI@short@VacuumPermeability}{% \ensuremath{% -8.85% -\times 10^{-12}\N\Amp^{-2}}} +1.26% +\times 10^{-6}\N\Amp^{-2}}} % \end{macrocode} % \end{macro} % @@ -5055,18 +10981,19 @@ %<*package> %\fi % \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: CODATA~2018 +% Source: Calculated % % \begin{macrocode} \DeclareRobustCommand{\k@SI@full@VacuumPermeability}{% \ensuremath{% -8.854\expandafter\physconst@decimalsseparator% -187\expandafter\physconst@decimalsseparator% -812\expandafter\physconst@decimalsseparator% -8% -\times 10^{-12}\N\Amp^{-2}}} +1.256\expandafter\physconst@decimalsseparator% +637\expandafter\physconst@decimalsseparator% +062\expandafter\physconst@decimalsseparator% +1% +\times 10^{-6}\N\Amp^{-2}}} % \end{macrocode} % \end{macro} % @@ -5077,9 +11004,10 @@ %<*package> %\fi % \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: CODATA~2018 +% Source: Calculated % % \begin{macrocode} \DeclareRobustCommand{\k@cgs@short@VacuumPermeability}{% @@ -5096,9 +11024,10 @@ %<*package> %\fi % \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: CODATA~2018 +% Source: Calculated % % \begin{macrocode} \DeclareRobustCommand{\k@cgs@full@VacuumPermeability}{% @@ -5118,6 +11047,7 @@ %<*package> %\fi % \begin{macro}{\kVacuumPermeability} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\kVacuumPermeability| is the magnetic permeability of the vacuum. % % \begin{macrocode} @@ -5147,6 +11077,113 @@ %\iffalse %<*package> %\fi +% \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@VacuumPermeabilityNumeric}{% +\ensuremath{% +1.26e-06}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@VacuumPermeabilityNumeric}{% +\ensuremath{% +1.2566370621e-06}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@VacuumPermeabilityNumeric}{% +\ensuremath{% +1.26e+01}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@VacuumPermeabilityNumeric}{% +\ensuremath{% +1.2566370614e+01}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kVacuumPermeabilityNumeric}{% +\k@SI@short@VacuumPermeabilityNumeric} +\else +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@SI@full@VacuumPermeabilityNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@cgs@short@VacuumPermeabilityNumeric} +\else +\DeclareRobustCommand {\kVacuumPermeabilityNumeric}{% +\k@cgs@full@VacuumPermeabilityNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \begin{macro}{\k@short@VacuumImpedance} % |\k@short@VacuumImpedance| is the characteristic impedance of the vacuum with % reduced precision. @@ -5208,6 +11245,62 @@ %\iffalse %<*package> %\fi +% \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@short@VacuumImpedanceNumeric}{% +\ensuremath{% +3.77e+02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@full@VacuumImpedanceNumeric}{% +\ensuremath{% +3.76730313668e+02}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kVacuumImpedanceNumeric} +% |\kVacuumImpedanceNumeric| is the characteristic impedance of the vacuum. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\kVacuumImpedanceNumeric}{% +\k@short@VacuumImpedanceNumeric} +\else +\DeclareRobustCommand {\kVacuumImpedanceNumeric}{% +\k@full@VacuumImpedanceNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \begin{macro}{\k@SI@short@Boltzmann} % |\k@SI@short@Boltzmann| is the Boltzmann constant in SI units with reduced % precision. @@ -5374,7 +11467,165 @@ %\iffalse %<*package> %\fi +% \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@short@BoltzmannNumeric}{% +\ensuremath{% +1.38e-23}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@SI@full@BoltzmannNumeric}{% +\ensuremath{% +1.380649e-23}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@short@BoltzmannNumeric}{% +\ensuremath{% +1.38e-16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@cgs@full@BoltzmannNumeric}{% +\ensuremath{% +1.380649e-16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@eV@short@BoltzmannNumeric}{% +\ensuremath{% +8.62e-05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@eV@full@BoltzmannNumeric}{% +\ensuremath{% +8.617333e-05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\kBoltzmannNumeric} +% |\kBoltzmannNumeric| is the Boltzmann constant. +% +% \begin{macrocode} +\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} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \begin{macro}{\keVBoltzmannNumeric} +% |\keVBoltzmannNumeric| is the Boltzmann constant. +% +% \begin{macrocode} +\ifx\shortconst\undefined +\DeclareRobustCommand {\keVBoltzmannNumeric}{% +\k@eV@short@BoltzmannNumeric} +\else +\DeclareRobustCommand {\keVBoltzmannNumeric}{% +\k@eV@full@BoltzmannNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \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 @@ -5394,6 +11645,7 @@ %<*package> %\fi % \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 % @@ -5414,6 +11666,7 @@ %<*package> %\fi % \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 @@ -5433,6 +11686,7 @@ %<*package> %\fi % \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 % @@ -5453,6 +11707,7 @@ %<*package> %\fi % \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 % @@ -5471,6 +11726,7 @@ %<*package> %\fi % \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 % @@ -5491,6 +11747,7 @@ %<*package> %\fi % \begin{macro}{\kPlanck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % |\kPlanck| is the Planck constant. % % \begin{macrocode} @@ -5521,6 +11778,7 @@ %<*package> %\fi % \begin{macro}{\keVPlanck} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % |\keVPlanck| is the Planck constant. % % \begin{macrocode} @@ -5540,7 +11798,170 @@ %\iffalse %<*package> %\fi +% \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@PlanckNumeric}{% +\ensuremath{% +6.63e-34}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckNumeric}{% +\ensuremath{% +6.62607015e-34}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckNumeric}{% +\ensuremath{% +6.63e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckNumeric}{% +\ensuremath{% +6.62607015e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckNumeric}{% +\ensuremath{% +4.14e-15}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckNumeric}{% +\ensuremath{% +4.13566770e-15}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kPlanckNumeric}{% +\k@SI@short@PlanckNumeric} +\else +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@SI@full@PlanckNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@cgs@short@PlanckNumeric} +\else +\DeclareRobustCommand {\kPlanckNumeric}{% +\k@cgs@full@PlanckNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\keVPlanckNumeric}{% +\k@eV@short@PlanckNumeric} +\else +\DeclareRobustCommand {\keVPlanckNumeric}{% +\k@eV@full@PlanckNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \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 @@ -5560,6 +11981,7 @@ %<*package> %\fi % \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 @@ -5581,6 +12003,7 @@ %<*package> %\fi % \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 @@ -5600,6 +12023,7 @@ %<*package> %\fi % \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 @@ -5621,6 +12045,7 @@ %<*package> %\fi % \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 @@ -5640,6 +12065,7 @@ %<*package> %\fi % \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 @@ -5661,6 +12087,7 @@ %<*package> %\fi % \begin{macro}{\kPlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % |\kPlanckReduced| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$. % @@ -5692,6 +12119,7 @@ %<*package> %\fi % \begin{macro}{\keVPlanckReduced} +% \changes{v1.1.0}{2020/02/03}{Fix order of magnitude of constant.} % |\keVPlanckReduced| is the Reduced Planck constant % $\left(\frac{h}{2\pi}\right)$. % @@ -5712,7 +12140,176 @@ %\iffalse %<*package> %\fi +% \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@PlanckReducedNumeric}{% +\ensuremath{% +1.05e-34}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckReducedNumeric}{% +\ensuremath{% +1.05457182e-34}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckReducedNumeric}{% +\ensuremath{% +1.05e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckReducedNumeric}{% +\ensuremath{% +1.05457182e-27}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckReducedNumeric}{% +\ensuremath{% +6.58e-16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@PlanckReducedNumeric}{% +\ensuremath{% +6.58211957e-16}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kPlanckReducedNumeric}{% +\k@SI@short@PlanckReducedNumeric} +\else +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@SI@full@PlanckReducedNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@cgs@short@PlanckReducedNumeric} +\else +\DeclareRobustCommand {\kPlanckReducedNumeric}{% +\k@cgs@full@PlanckReducedNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\keVPlanckReducedNumeric}{% +\k@eV@short@PlanckReducedNumeric} +\else +\DeclareRobustCommand {\keVPlanckReducedNumeric}{% +\k@eV@full@PlanckReducedNumeric} +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*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 @@ -5791,6 +12391,7 @@ %<*package> %\fi % \begin{macro}{\kGravity} +% \changes{v1.1.0}{2020/02/03}{Fix value of constant.} % |\kGravity| is Newton's gravitational constant. % % \begin{macrocode} @@ -5820,7 +12421,115 @@ %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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. @@ -5830,7 +12539,7 @@ \DeclareRobustCommand{\k@SI@short@StefanBoltzmann}{% \ensuremath{% 5.67% -\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} +\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -5841,6 +12550,7 @@ %<*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. @@ -5851,7 +12561,7 @@ \ensuremath{% 5.670\expandafter\physconst@decimalsseparator% 374% -\times 10^{-6}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} +\times 10^{-8}\J\Kelvin^{-4}\m^{-2}\Sec^{-1}}} % \end{macrocode} % \end{macro} % @@ -5862,6 +12572,7 @@ %<*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. @@ -5882,6 +12593,7 @@ %<*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. @@ -5903,6 +12615,7 @@ %<*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 % $\left(\frac{2\pi^5k_\mathrm{B}}{15h^3c^2}\right)$. % @@ -5933,6 +12646,118 @@ %\iffalse %<*package> %\fi +% \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@StefanBoltzmannNumeric}{% +\ensuremath{% +5.67e-08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@StefanBoltzmannNumeric}{% +\ensuremath{% +5.670374e-08}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@StefanBoltzmannNumeric}{% +\ensuremath{% +5.67e-05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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@StefanBoltzmannNumeric}{% +\ensuremath{% +5.670374e-05}} +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi +% \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 {\kStefanBoltzmannNumeric}{% +\k@SI@short@StefanBoltzmannNumeric} +\else +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@SI@full@StefanBoltzmannNumeric} +\fi +\else +\ifx\shortconst\undefined +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@cgs@short@StefanBoltzmannNumeric} +\else +\DeclareRobustCommand {\kStefanBoltzmannNumeric}{% +\k@cgs@full@StefanBoltzmannNumeric} +\fi +\fi +% \end{macrocode} +% \end{macro} +% +%\iffalse +%</package> +%\fi +%\iffalse +%<*package> +%\fi % \begin{macro}{\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 @@ -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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\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 %</package> %\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 +%</package> +%\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 +%</package> +%\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 +%</package> +%\fi % \CheckSum{0} % \Finale \makeatother |