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).