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author | jthorn <jthorn@e296648e-0e4f-0410-bd07-d597d9acff87> | 2005-01-24 13:52:39 +0000 |
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committer | jthorn <jthorn@e296648e-0e4f-0410-bd07-d597d9acff87> | 2005-01-24 13:52:39 +0000 |
commit | 85844140ed2ab79769e342f21e4fad20cedd60f9 (patch) | |
tree | 8974b98a9f79423b48f59a823cf3910159598c7e /doc | |
parent | 5a76904aa9e3fd70ae74f2e9e81f196d107b38de (diff) |
fix undefined reference
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/Exact/trunk@214 e296648e-0e4f-0410-bd07-d597d9acff87
Diffstat (limited to 'doc')
-rw-r--r-- | doc/documentation.tex | 5 |
1 files changed, 3 insertions, 2 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex index 84dd3f5..b6da738 100644 --- a/doc/documentation.tex +++ b/doc/documentation.tex @@ -969,8 +969,9 @@ version of the Friedmann-Robertson-Walker model with flat space linear dependence between the energy density $\epsilon$ and the pressure, $p$, namely $p=\kappa \epsilon$. Thus the metric is the Robertson-Walker metric -(see section~\ref{AEIThorns/Exact/sect-Robertson-Walker}) with -$k =0$ and (see gr-qc/0110030, astro-ph/9910093 and references cited here) +%%(see section~\ref{AEIThorns/Exact/sect-Robertson-Walker}) +with $k =0$ and (see gr-qc/0110030, astro-ph/9910093 and references +cited here), \begin{equation} R(t) = R_0 \left[ \cosh \left(\frac{\sqrt{3\Lambda}}{2}(\kappa+1) t \right) + |