documentation.tex: Add braces for htlatex

git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEOS/EOS_Omni/trunk@51 8e189c6b-2ab8-4400-aa02-70a9cfce18b9

1 files changed, 5 insertions, 5 deletions

diff --git a/doc/documentation.tex b/doc/documentation.tex
index c0b1f77..743c472 100644
--- a/doc/documentation.tex
+++ b/doc/documentation.tex
@@ -305,14 +305,14 @@ simulations of stellar collapse to mimic (1) the stiffening of the
 nuclear EOS at nuclear density and (2) to include thermal pressure in
 the postbounce phase.  It consists of two polytropes characterized by
 ($K_1$, $\gamma_1$) and ($K_2$, $\gamma_2$) and a thermal $\gamma-$law
-component described by $\gamma_\mathrm{th}$.  Polytrope 1 is soft and
+component described by $\gamma_{\mathrm{th}}$.  Polytrope 1 is soft and
 describes a gas of relativistic degenerate electrons with $\gamma_1
-\approx 4/3$.  It is used below nuclear density ($\rho_\mathrm{nuc}
+\approx 4/3$.  It is used below nuclear density ($\rho_{\mathrm{nuc}}
 \approx 2\times10^{14}\,\mathrm{g\,cm}^{-3}$), and is smoothly matched to
-polytrope 2 which applies above $\rho_\mathrm{nuc}$, is stiff, and
+polytrope 2 which applies above $\rho_{\mathrm{nuc}}$, is stiff, and
 models the repulsive core of the strong force above nuclear density
 ($\gamma_2 \gtrsim 2.5$).  $K_2$ is completely determined by
-$P_1(\rho_\mathrm{nuc}) = P_2(\rho_\mathrm{nuc})$ and $K_1, \gamma_1,$
+$P_1(\rho_{\mathrm{nuc}}) = P_2(\rho_{\mathrm{nuc}})$ and $K_1, \gamma_1,$
 and $\gamma_2$. The full functional form of the EOS
 $P=P(\rho,\epsilon)$ with the thermal component (which takes into
 account shock heating) is given by
@@ -331,7 +331,7 @@ The \texttt{EOS\_Omni} parameters for the hybrid EOS are the following:
 \begin{tabular}{ll}
 \texttt{hybrid\_gamma1}     & $\gamma_1$,  $\gamma_1 = 1.325$ is an appropriate choice.\\
 \texttt{hybrid\_gamma2}     & $\gamma_2$,  $\gamma_2 = 2.5$ is an appropriate choice.\\
-\texttt{hybrid\_gamma\_th}   & $\gamma_\mathrm{th}$, perhaps $1.5$.\\
+\texttt{hybrid\_gamma\_th}   & $\gamma_{\mathrm{th}}$, perhaps $1.5$.\\
 \texttt{hybrid\_k1}         & $K_1$, $0.4640517$ in solar units for relativistic degenerate e$^{-}$.\\
 \texttt{hybrid\_rho\_nuc}    & nuclear density, standard is $3.238607\times 10^{-4}$ in solar units.
 \end{tabular}