[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 4)

[knarf at cct.lsu.edu]

User: knarf
Date: 2011/01/17 09:55 AM

Modified:
 /
  ET.tex

Log:
 change structure a bit

File Changes:

Directory: /
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File [modified]: ET.tex
Delta lines: +41 -24
===================================================================
--- ET.tex	2010-12-14 21:49:21 UTC (rev 3)
+++ ET.tex	2011-01-17 15:55:53 UTC (rev 4)
@@ -59,7 +59,7 @@
 B. Giacomazzo,	T. Goodale, C. Gundlach,  R. Haas, I. Hawke, S. Hawley,     I. Hinder, T. Kellermann,
 G. Lanfermann,   F. L\"{o}ffler$^{(3)}$, J. Masso, M. Miller, P. Montero,  C. Ott,
   R. Paruchuri$^{(3)}$, D. Pollney, T. Radke, L. Rezzolla, D. Rideout, M. Ripeanu, E. Schnetter$^{(2,3)}$,
-E. Seidel, E. L. Seidel, J. Shalf, N. Stergioulas, R. Takahashi, J. Thornburg, A. Tonita, P. Walker}
+E. Seidel, E. L. Seidel, J. Shalf, N. Stergioulas, R. Takahashi, J. Thornburg, A. Tonita, P. Walker\textbf{check, sort}}
 
 
 \thanks{{}$^{(1)}$ Department of Computer Science,
@@ -84,9 +84,13 @@
 
 \section{Introduction}
 
-Scientific progress in the field of numerical relativity has always been closely tied with the availability and ease-of-use of enabling software and computational infrastructure. This document describes the Einstein Toolkit. 
+Scientific progress in the field of numerical relativity has always
+been closely tied with the availability and ease-of-use of enabling
+software and computational infrastructure. This document describes
+the Einstein Toolkit, which aims at providing such an infrastructure,
+developed openly and available freely.
 
-This is a particularly exciting time for numerical relativity and
+Now is a particularly exciting time for numerical relativity and
 relativistic astrophysics. Recent computational
 breakthroughs~\cite{Pretorius:2005gq, Campanelli:2005dd, Baker:2005vv}
 have transformed the field with our ability to
@@ -137,8 +141,8 @@
 collaborators, including co-PI Faber, e.g.,
 \cite{Etienne:2007jg,Liu:2008xy}), LSU (Lehner et al.,
 \cite{Anderson:2007kz,Anderson:2008zp}), Caltech-Cornell (Duez et
-al.~\cite{Duez:2008rb}), and at the AEI~(Rezzolla and collaborators,
-\cite{Baiotti:2008ra,loeffler:06}).  The first simulations in 3D GRHD
+al.~\cite{Duez:2008rb}), and at the AEI and Sissa~(Rezzolla and collaborators,
+\cite{Baiotti:2008ra,Loeffler06a}).  The first simulations in 3D GRHD
 of massive star collapse to protoneutron stars have been carried out
 by co-PI Ott and collaborators \cite{ott:07prl,ott:07cqg} and by
 Shibata~et~al.~\cite{shibata:053D}. The collapse of rotating,
@@ -223,11 +227,9 @@
 \subsection{Academic and Social}
 
 \begin{itemize}
-
-\item A primary concern for research groups is securing reliable funding to maintain graduate students and postdoctoral researchers. 
-
+\item A primary concern for research groups is securing reliable funding
+      to maintain graduate students and postdoctoral researchers. 
 \item 
-
 \end{itemize}
 
 \section{Design and Strategy for the Einstein Toolkit}
@@ -257,7 +259,7 @@
 application domains.
 
 
-\subsection{Carpet}
+\subsection{Carpet Mesh Refinement}
 
 While Cactus is distributed with a structured-mesh unigrid MPI
 parallel driver (\codename{PUGH}\footnote{Recent results with a
@@ -279,10 +281,20 @@
 source and is openly developed, with the main development located at
 LSU (co-PI Schnetter) and contributions from AEI and others.
 
+\subsection{CactusEinstein} The Cactus Framework was developed by the
+numerical relativity community, and although it is a general component
+framework that supports different application domains its core user
+group has remained from numerical relativity. The Cactus Team have
+traditionally developed and supported a set of core modules for numerical
+relativity, as part of the {\tt CactusEinstein} arrangement. Over the
+last few years however, the relevance of many of the modules has declined,
+and more and more of the basic infrastructure for numerical relativity
+has been provided by open modules provided and distributed by research
+groups in the community. 
 
+The Einstein Toolkit collects the widely used parts of CactusEinstein,
+combined with contributions from the community.
 
-\subsection{CactusEinstein} The Cactus Framework was developed by the numerical relativity community, and although it is a general component framework that supports different application domains its core user group has remained from numerical relativity. The Cactus Team have traditionally developed and supported a set of core modules for numerical relativity, as part of the {\tt CactusEinstein} arrangement. Over the last few years however, the relevance of many of the modules has declined, and more and more of the basic infrastructure for numerical relativity has been provided by open modules provided and distributed by research groups in the community. 
-
 \subsection{Whisky Code}
 
 \subsection{Simulation Factory}
@@ -291,27 +303,31 @@
 
 
 
+\section{Components}
 
+\subsection{Base Modules}
 
+\paragraph{Vacuum Spacetimes}
 
-\section{Components}
+\paragraph{Relativistic Matter Spacetimes}
 
-\subsection{Vacuum Spacetimes}
 
-\subsection{Relativistic Matter Spacetimes}
-
-\subsection{Gauge Conditions}
-
 \subsection{Initial Data}
 
 \paragraph{Gravitational Waves}
 
-\paragraph{Black Hole}
+\paragraph{Black Holes}
 
-\paragraph{Perturbed Black Hole}
-
 \paragraph{Neutron Stars}
 
+
+\subsection{Evolution Methods}
+
+\paragraph{Spacetime}
+
+\paragraph{Relativistic Matter}
+
+
 \subsection{Analysis}
 
 \paragraph{Masses}
@@ -320,13 +336,15 @@
 
 \paragraph{Gravitational Waves}
 
+
 \subsection{Relativity Tools}
 
 \paragraph{Black Hole Excision}
 
-
 \paragraph{Vacuum-Matter Coupling}
 
+\paragraph{Object tracking}
+
 \subsection{Numerical Methods}
 
 \paragraph{Domains and Coordinates}
@@ -336,10 +354,9 @@
 \paragraph{Boundary Conditions}
 
 
-
 \section{Examples}
 
-kerr-schild, binary, TOV
+kerr-schild, BH-binary, TOV
 
 \section{Results}