[Commits] [svn:einsteintoolkit] EOS_Omni/trunk/doc/ (Rev. 46)

[schnetter at cct.lsu.edu]

User: eschnett
Date: 2011/04/19 07:59 PM

Modified:
 /trunk/doc/
  documentation.tex

Log:
 Some grammar corrections

File Changes:

Directory: /trunk/doc/
======================

File [modified]: documentation.tex
Delta lines: +8 -8
===================================================================
--- trunk/doc/documentation.tex	2011-04-20 00:39:48 UTC (rev 45)
+++ trunk/doc/documentation.tex	2011-04-20 00:59:23 UTC (rev 46)
@@ -112,11 +112,11 @@
 
 \begin{abstract}
   \noindent This thorn provides a unified EOS (Equation Of State)
-  interface and implements multiple analytic EOS and provides table
+  interface and implements multiple analytic EOS, and also provides table
   reader and interpolation routines for finite-temperature
-  microphysical EOS available from {\tt
-    http://www.stellarcollapse.org}\@. Currently, the implemented
-  analytic EOS are the polytropic EOS, the gamma-law EOS, a hybrid EOS
+  microphysical EOS available from
+    \url{http://www.stellarcollapse.org}. Currently, the implemented
+  analytic EOS are the polytropic EOS, the gamma-law EOS, and a hybrid EOS
   consisting of a 2-piece piecewise-polytrope with an a thermal,
   gamma-law component.
 \end{abstract}
@@ -150,7 +150,7 @@
 
 \texttt{EOS\_Omni} works via the aliased-function interface, and
 EOS functions to be used must be declared in \texttt{interface.ccl}.
-Here is an example call/{interface.ccl} entry:
+Here is an example \texttt{interface.ccl} entry:
 \begin{verbatim}
 void FUNCTION EOS_Omni_press(CCTK_INT IN eoskey,         \
                              CCTK_INT IN havetemp,       \
@@ -176,7 +176,7 @@
     \item \texttt{eoskey = 4}: Finite-temperature microphysical EOS
   \end{itemize}
 \item \texttt{havetemp} determines whether the EOS is to be called as
-  a function of $(\rho,\epsilon,Y_e)$ (\texttt{havetemp = 0}), as a
+  a function of $(\rho,\epsilon,Y_e)$ (\texttt{havetemp = 0}), or as a
   function of $(\rho,T,Y_e)$ (\texttt{havetemp = 1}).
   \texttt{havetemp = 0} is the method of choice for analytic EOS during
   evolution, but at the initial data stage one may need to set
@@ -249,7 +249,7 @@
 \end{eqnarray}
 (which actually ignores the temperature).
 
-Internally, \texttt{EOS\_Omni} uses cgs units and on startup converts
+Internally, \texttt{EOS\_Omni} uses cgs units, and on startup converts
 the EOS parameters from solar units to cgs units. This conversion
 depends on $\gamma$ and the value of $\gamma$ at the initial
 data stage (\texttt{poly\_gamma\_ini}) is used for this.
@@ -310,7 +310,7 @@
 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 ($\rho_\mathrm{nuc}
-\approx 2\times10^{14}\,\mathrm{g\,cm}^{-3}$) and smoothly matched to
+\approx 2\times10^{14}\,\mathrm{g\,cm}^{-3}$), and is smoothly matched to
 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