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authorjthorn <jthorn@e296648e-0e4f-0410-bd07-d597d9acff87>2005-01-24 13:52:39 +0000
committerjthorn <jthorn@e296648e-0e4f-0410-bd07-d597d9acff87>2005-01-24 13:52:39 +0000
commit85844140ed2ab79769e342f21e4fad20cedd60f9 (patch)
tree8974b98a9f79423b48f59a823cf3910159598c7e /doc
parent5a76904aa9e3fd70ae74f2e9e81f196d107b38de (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.tex5
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)
+