[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 35)

knarf at cct.lsu.edu knarf at cct.lsu.edu
Tue Mar 22 09:55:47 CDT 2011 

User: knarf
Date: 2011/03/22 09:55 AM

Modified:
 /
  ET.tex

Log:
 add comments with names and length to sections

File Changes:

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

File [modified]: ET.tex
Delta lines: +37 -54
===================================================================
--- ET.tex	2011-03-14 15:08:29 UTC (rev 34)
+++ ET.tex	2011-03-22 14:55:47 UTC (rev 35)
@@ -29,7 +29,9 @@
 \def\gt#1{Georgia Tech#1 (GaTech#1)\gdef\gt{GaTech}}
 
 \newcommand{\codename}[1]{\texttt{#1}}
-\newcommand{\todo}[1]{{\color{blue}$\blacksquare$~\textsf{[TODO: #1]}}}
+\newcommand{\todo}[1]{{\color{red}$\blacksquare$~\textsf{[TODO: #1]}}}
+\newcommand{\comment}[1]{{\color{blue}$\blacksquare$~\textsf{[Comment: #1]}}}
+\newcommand{\pages}[1]{{\color{blue}$\blacksquare$~\textsf{[#1]}}}
 
 % Don't use tt font for urls
 \urlstyle{rm}
@@ -69,19 +71,16 @@
 
 
 
-\thanks{{}$^{(1)}$ Department of Computer Science,
-  Louisiana State University, Baton Rouge, LA 70803, USA}
+%\thanks{{}$^{(1)}$ Department of Computer Science,
+%  Louisiana State University, Baton Rouge, LA 70803, USA}
+%\thanks{{}$^{(2)}$ Department of Physics \& Astronomy,
+%  Louisiana State University, Baton Rouge, LA 70803, USA}
+%\thanks{{}$^{(3)}$ Center for Computation \& Technology,
+%  Louisiana State University, Baton Rouge, LA 70803, USA}
+%\thanks{{}$^{(4)}$ Center for Computational Relativity \& Gravitation,
+%  School of Mathematical Sciences,
+%  Rochester Institute of Technology, Rochester, New York 14623, USA}
 
-\thanks{{}$^{(2)}$ Department of Physics \& Astronomy,
-  Louisiana State University, Baton Rouge, LA 70803, USA}
-
-\thanks{{}$^{(3)}$ Center for Computation \& Technology,
-  Louisiana State University, Baton Rouge, LA 70803, USA}
-
-\thanks{{}$^{(4)}$ Center for Computational Relativity \& Gravitation,
-  School of Mathematical Sciences,
-  Rochester Institute of Technology, Rochester, New York 14623, USA}
-
 % TODO: Already add a few affiliations which we know are going
 %       to be used
     
@@ -91,8 +90,11 @@
 
 \maketitle
 
+% We will remove this at the end, but we leave it in for ourselfes now
+\tableofcontents
 
-\section{Introduction}
+\section{Introduction\pages{1 Frank}}
+\comment{About 1 page}
 
 Scientific progress in the field of numerical relativity has always
 been closely tied with the availability and ease-of-use of enabling
@@ -168,7 +170,7 @@
 
  
 
-\section{Requirements}
+\section{Requirements\pages{2 Frank}}
 
 \subsection{Scientific}
 
@@ -246,7 +248,7 @@
 other areas of science and hereby providing an immediate application
 of their research.
 
-\section{Design and Strategy for the Einstein Toolkit}
+\section{Design and Strategy\pages{1 Frank}}
 
 The mechanisms for the development and support of the Einstein Toolkit are
 designed to be open, transparent and community driven. All the source code,
@@ -274,10 +276,9 @@
 Einstein Toolkit Maintainer, and is generally open for discussion on the
 users mailing list.
 
-\section{Core Technologies}
+\section{Core Technologies\pages{0.5 Frank}}
 
-\subsection{Cactus Framework}
-\todo{1/2 page Gab}
+\subsection{Cactus Framework\pages{1 Gab}}
 
 The \textbf{Cactus
   Framework}~\cite{CS_cactus_web,CS_Goodale02a,CS_cactususersguide} is
@@ -311,7 +312,7 @@
 The Einstein Toolkit now collects the widely used parts of CactusEinstein,
 combined with contributions from the community.
 
-\subsection{Adaptive Mesh Refinement}
+\subsection{Adaptive Mesh Refinement\pages{1 Erik}}
 
 \todo{ES: add/check citations}
 \todo{ES: remove names}
@@ -354,7 +355,7 @@
 % E. Schnetter \todo{ES: do we want names here?} and is funded via several
 % NSF awards \todo{ES: list them somewhere}.
 
-\subsection{Simulation Factory}
+\subsection{Simulation Factory\pages{1 Erik/Michael}}
 
 It is unfortunate that today's supercomputers differ significantly in
 their hardware configuration, available software, directory structure,
@@ -386,8 +387,7 @@
 The exact same set of commands can be used on all other supported
 supercomputers to run the same simulation there.
 
-\subsection{Kranc}
-\todo{1/3 page Ian}
+\subsection{Kranc\pages{1 Ian}}
 
 Kranc\cite{Husa:2004ip,kranc04,krancweb} is a Mathematica application which converts a high-level
 continuum description of a PDE into a highly optimised module for
@@ -424,9 +424,9 @@
 as well as the wave extraction thorn WeylScal4, are both generated
 using Kranc, and hence support all the above features.
 
-\section{Components}
+\section{Components\pages{0.5 Frank}}
 
-\subsection{Base Modules}
+\subsection{Base Modules\pages{4 Frank}}
 \label{sec:base_modules}
 Modular designs have proven to be essential for distributed development
 of complex software systems, and require the use of well defined interfaces.
@@ -485,8 +485,7 @@
 to the Faraday tensor and the unit normal of the foliation of spacetime
 $n^\mu$.
 
-\subsection{Initial Data}
-\todo{1/2 page Josh, Bruno}
+\subsection{Initial Data\pages{4 Josh/Bruno}}
 The Einstein Toolkit contains many modules used to generate initial data for 
 general relativistic simulations, including both vacuum and hydrodynamical
 configurations.  
@@ -543,16 +542,14 @@
 the \codename{TwoPunctures} module can also be used to construct neutron star
 black hole binary initial data, when being coupled with \codename{TOVSolver}.
 
-\subsection{Evolution Methods}
-\todo{1/2 page Christian}
+\subsection{Evolution Methods\pages{4 Christian}}
 
 \paragraph{Spacetime}
 
 \paragraph{Relativistic Matter}
 
 
-\subsection{Analysis}
-%\todo{1/2 page Tanja}
+\subsection{Analysis\pages{4 Tanja}}
 
 Any simulated system may have many applicable quantities for analysis which 
 are most efficiently calculated during evolution.  The Einstein Toolkit 
@@ -589,8 +586,7 @@
 Weyl scalars, as well as any other quantity, can be projected onto a basis 
 of spin-weighted spherical harmonics using the \codename{Multipole} module.
 
-\subsection{Relativity Tools}
-\todo{1/2 page Peter}
+\subsection{Relativity Tools\pages{3 Peter}}
 
 \paragraph{Black Hole Excision}
 
@@ -621,8 +617,7 @@
 
 
 
-%\subsection{Infrastructure and Numerical Methods}
-\subsection{Simulation Domain, Symmetries, Boundaries}
+\subsection{Simulation Domain, Symmetries, Boundaries\pages{3 Roland?}}
 
 \paragraph{Domains and Coordinates.}
 The simulation domain is specified via the parameter file \todo{ES:
@@ -671,36 +666,24 @@
 
 
 
-\section{Examples}
-\todo{2 pages in total, 1 plot per paragraph, Frank coordinates}
+\section{Examples\pages{0.5 Frank}}
 
-\paragraph{Kerr-Schild}
-\todo{1/2 page, Bruno}
-Show stable Kerr-evolution. What is commonly shown for this nowadays, the
-spectrum of the ringdown of a perturbation?
+\subsection{Vacuum\pages{2 Bruno}}
 
-\paragraph{BH-binary}
-\todo{1/2 page, Peter}
-Show binary merger and plot of waveform in either time or frequency domain.
+\subsection{TOV\pages{2 Frank}}
+Show stable TOV evolution
 
-\paragraph{TOV+mEOS}
-\todo{1/2 page, Frank}
-Show stable TOV evolution, once with Polytropes and once with mEOS,
-both including oscillation spectra
-
-\paragraph{Collapse}
-\todo{1/2 page, Frank, Christian}
+\subsection{Collapse\pages{2 Christian}}
 Show TOV collapse and BH formation
 
 
-\section{Future Work}
-\todo{Frank}
+\section{Future Work\pages{1 Frank}}
 - MHD
 - massively parallel AMR
 - radiation transport
 - advanced wave extraction
 
-\section*{Acknowledgments}
+\section*{Acknowledgments\pages{0.5 All}}
 \todo{Frank, ADDME}
 The Einstein Toolkit is directly supported by the National Science Foundation
 under the grant numbers 0903973/0903782/0904015 (CIGR).

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