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}