diff options
author | Norbert Preining <norbert@preining.info> | 2022-10-11 03:01:16 +0000 |
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committer | Norbert Preining <norbert@preining.info> | 2022-10-11 03:01:16 +0000 |
commit | 2713ec666b0e53418a839b97c48e0a9234fe5c98 (patch) | |
tree | 44f44c40d7cf3d6c2c0be9da7bfcf4dad97eb483 /macros/latex/contrib/exam-n/sample/cosmo3.tex | |
parent | 9c7942efff8183c8695ec824008847dd068dbfe7 (diff) |
CTAN sync 202210110301
Diffstat (limited to 'macros/latex/contrib/exam-n/sample/cosmo3.tex')
-rw-r--r-- | macros/latex/contrib/exam-n/sample/cosmo3.tex | 4 |
1 files changed, 2 insertions, 2 deletions
diff --git a/macros/latex/contrib/exam-n/sample/cosmo3.tex b/macros/latex/contrib/exam-n/sample/cosmo3.tex index b7b74c0107..aa3f78868a 100644 --- a/macros/latex/contrib/exam-n/sample/cosmo3.tex +++ b/macros/latex/contrib/exam-n/sample/cosmo3.tex @@ -32,7 +32,7 @@ equivalent to an empty, flat, Universe with a non-zero $\Lambda$. of state with $w = 0$ for $0 < t < t_0$, but which changes to $W=0$ for $t\ge t_0$ without any discontinuity in $H(t)$. Regarding this second stage as driven by a non-zero $\Lambda$ what -is the value of $\Lambda$ if $t_0 = 10^{24}$\units{\mu s}? Define the +is the value of $\Lambda$ if $t_0 = \SI{1e24}{\mu s}$? Define the dimensionless deceleration parameter, $q$, and find its value before and after $t_0$. \shout{Shout it loud: I'm a geek and I'm proud} @@ -40,7 +40,7 @@ before and after $t_0$. Note: that's \[ -t_0=10^{24}\units{\mu s}\qquad\text{with a letter mu: $\mu$}. +t_0=\SI{1e24}{\mu s}\qquad\text{with a letter mu: $\mu$}. \] \part To what extent does this idealized model resemble the currently |