[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 305)

[knarf at cct.lsu.edu]

User: knarf
Date: 2012/03/13 09:41 AM

Modified:
 /
  ET.tex

Log:
 don't use 'ET' within the paper

File Changes:

Directory: /
============

File [modified]: ET.tex
Delta lines: +2 -2
===================================================================
--- ET.tex	2012-03-13 14:40:26 UTC (rev 304)
+++ ET.tex	2012-03-13 14:41:35 UTC (rev 305)
@@ -696,7 +696,7 @@
 \label{table:vars}
 {\centering
 \begin{tabular}{llll}
-Symbol & Quantity & Eqn. & ET thorn::group \\
+Symbol & Quantity & Eqn. & Einstein Toolkit thorn::group \\
 \hline
 $G_{\mu\nu}$ & Einstein Tensor & \protect\ref{eq:einstein} & N/A\\
 $T_{\mu\nu}$ & Stress-Energy Tensor & \protect\ref{eq:Tmunu} & TmunuBase::stress\_energy\_tensor\\
@@ -1111,7 +1111,7 @@
 
 \subsubsection{TOVSolver}
 \label{sec:TOVSolver}
-The \codename{TOVSolver} routine in the ET solves the standard TOV equations 
+The \codename{TOVSolver} routine in the Einstein Toolkit solves the standard TOV equations 
 \cite{Tolman:1939jz,Oppenheimer:1939ne} for the pressure, enclosed gravitational mass $M_e$, and gravitational potential $\Phi=\log\alpha$  in the interior of a spherically symmetric star in hydrostatic equilibrium, expressed using the Schwarzschild (areal) 
 radius $\hat{r}$:
 \begin{eqnarray}