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}}