User: knarf Date: 2011/11/14 09:57 AM

Modified: / ET.tex

Log: remove development macros

File Changes:

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

File [modified]: ET.tex Delta lines: +3 -11 =================================================================== --- ET.tex 2011-11-14 15:53:56 UTC (rev 217) +++ ET.tex 2011-11-14 15:57:11 UTC (rev 218) @@ -45,15 +45,7 @@ \newcommand{\todo}[1]{{\color{red}$\blacksquare$~\textsf{[TODO: #1]}}} %conflicting definition with iop packages %\newcommand{\comment}[1]{{\color{blue}$\blacksquare$~\textsf{[Comment: #1]}}} -\newcommand{\pages}[1]{{\color{blue}$\blacksquare$~\textsf{[#1]}}}

-% Use this macro for sections which are done, so that those comments -% can easily be disabled. -\newcommand{\pagesdone}[1]{{\color{green}$\blacksquare$~\textsf{[#1]}}} -%\newcommand{\pagesdone}[1]{} - -\newcommand{\BCM}[1]{{\bf \color{blue} [BCM: #1] }} %BCM comments - % Don't use tt font for urls \urlstyle{rm}

@@ -2545,7 +2537,7 @@ \label{fig:amp_phs_convergence} \end{figure}

-\subsection{Linear oscillations of TOV stars\pages{2 Frank}} +\subsection{Linear oscillations of TOV stars} \label{sec:tov_oscillations} The examples in the previous subsections did not include the evolution of matter within a relativistic spacetime. One interesting test of a coupled @@ -2650,7 +2642,7 @@ the stellar center and surface is higher than $1.5$, but mostly below $2$.} \end{figure}

-\subsection{Neutron star collapse\pages{2 Christian, Roland}} +\subsection{Neutron star collapse} \label{sec:collapse_example} The previous examples dealt either with preexisting BHs, either single or in a binary, or with a smooth singularity free spacetime, as in the @@ -2931,7 +2923,7 @@ generation of true petascale supercomputers on which typical compute jobs are expected to be running on 100,000 and more compute cores.

-\section*{Acknowledgments\pages{0.5 All}} +\section*{Acknowledgments} \todo{All: Add!} The Einstein Toolkit is directly supported by the National Science Foundation in the USA under the grant numbers