[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 84)

[knarf at cct.lsu.edu]

User: knarf
Date: 2011/05/09 10:48 AM

Modified:
 /
  ET.tex

Log:
 enable kasner example pics in tex

File Changes:

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

File [modified]: ET.tex
Delta lines: +11 -11
===================================================================
--- ET.tex	2011-05-09 15:11:56 UTC (rev 83)
+++ ET.tex	2011-05-09 15:48:54 UTC (rev 84)
@@ -1816,8 +1816,8 @@
 \label{sec:bbh-example}
 
 \subsection{TOV\pages{2 Frank}}
-Show stable TOV evolution
 
+
 \subsection{Collapse\pages{2 Christian}}
 Show TOV collapse and BH formation
 
@@ -1858,16 +1858,16 @@
 of spacetime~\ref{eq:kasner}, along with the associated error for a sequence of 
 time resolutions.
 
-%\begin{figure}
-%\includegraphics[width=0.45\textwidth]{kasner.png}
-%\includegraphics[width=0.45\textwidth]{err.png}
-%\caption{Left: the evolution of a vacuum spacetime of the type~\ref{eq:gowdyT3},
-%with $P=Q=\lambda=0$; the initial data are chosen as
-%$\gamma_{ij}=\delta_{ij}$ and $K_{ij}={\rm diag}(-2/3,-2/3,1/3)$.
-%Right: the numerical error for a sequence of four time resolutions $dt=[0.0125,0.025,0.05,0.1]$;
-%the errors are scaled according to the expectation for fourth-order convergence.
-%\label{fig:kasner}}
-%\end{figure}
+\begin{figure}
+ \includegraphics[width=0.45\textwidth]{kasner.png}
+ \includegraphics[width=0.45\textwidth]{err.png}
+ \caption{Left: the evolution of a vacuum spacetime of the type~\ref{eq:gowdyT3},
+ with $P=Q=\lambda=0$; the initial data are chosen as
+ $\gamma_{ij}=\delta_{ij}$ and $K_{ij}={\rm diag}(-2/3,-2/3,1/3)$.
+ Right: the numerical error for a sequence of four time resolutions $dt=[0.0125,0.025,0.05,0.1]$;
+ the errors are scaled according to the expectation for fourth-order convergence.
+ \label{fig:kasner}}
+\end{figure}
 
 
 \section{Future Work\pages{1 Frank}}