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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 226)
by schnetter＠cct.lsu.edu 14 Nov '11

14 Nov '11

User: eschnett Date: 2011/11/14 10:36 AM Modified: / ET.tex Log: Acknowledge people's contributions File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +8 -2 =================================================================== --- ET.tex 2011-11-14 16:35:28 UTC (rev 225) +++ ET.tex 2011-11-14 16:36:17 UTC (rev 226) @@ -2927,9 +2927,15 @@ are expected to be running on 100,000 and more compute cores. \section*{Acknowledgments} -\todo{All: Add!} The authors wish to thank Ed Seidel whose + +The authors wish to thank Ed Seidel whose inspiration and vision has driven work towards the Einstein Toolkit -over the past 15 years. The Einstein Toolkit is directly supported by +over the past 15 years. +We are also grateful to the large number of people who contributed to +the Einstein Toolkit via ideas, code, documentation, and testing; +without these contributions, this toolkit would not exist today. + +The Einstein Toolkit is directly supported by the National Science Foundation in the USA under the grant numbers 0903973/0903782/0904015 (CIGR\@). Related grants contribute directly and indirectly to the success of CIGR, including NSF OCI-0721915, NSF

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 225)
by jfaber＠einsteintoolkit.org 14 Nov '11

14 Nov '11

User: jfaber Date: 2011/11/14 10:35 AM Modified: / ET.tex Log: sort and compress refs, fix page heads File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +6 -2 =================================================================== --- ET.tex 2011-11-14 16:31:17 UTC (rev 224) +++ ET.tex 2011-11-14 16:35:28 UTC (rev 225) @@ -27,6 +27,9 @@ \usepackage[bookmarks, bookmarksopen, bookmarksnumbered]{hyperref} \usepackage[all]{hypcap} +\usepackage[sort&compress,numbers]{natbib} +\renewcommand{\bibfont}{\footnotesize} + \graphicspath{{figures/}} \setcounter{secnumdepth}{5} @@ -138,7 +141,7 @@ \maketitle % We will remove this at the end, but we leave it in for ourselves now -\tableofcontents +%\tableofcontents \section{Introduction} @@ -2949,7 +2952,8 @@ authors and do not necessarily reflect the views of the National Science Foundation. -\section*{References} +% Take this out when using natbib +%\section*{References} \bibliographystyle{iopart-num-edit} %\bibliographystyle{amsplain-url}

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 224)
by knarf＠cct.lsu.edu 14 Nov '11

14 Nov '11

User: knarf Date: 2011/11/14 10:31 AM Modified: / ET.tex Log: add gabs 'stub' in the ackn File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +8 -1 =================================================================== --- ET.tex 2011-11-14 16:29:10 UTC (rev 223) +++ ET.tex 2011-11-14 16:31:17 UTC (rev 224) @@ -42,7 +42,8 @@ \newcommand{\dfrac}[2]{{\frac{#1}{#2}}} \newcommand{\codename}[1]{\texttt{#1}} -\newcommand{\todo}[1]{{\color{red}$\blacksquare$~\textsf{[TODO: #1]}}} +%\newcommand{\todo}[1]{{\color{red}$\blacksquare$~\textsf{[TODO: #1]}}} +\newcommand{\todo}[1]{} %conflicting definition with iop packages %\newcommand{\comment}[1]{{\color{blue}$\blacksquare$~\textsf{[Comment: #1]}}} @@ -2942,6 +2943,12 @@ DE-AC03-76SF00098, at the Leibniz Rechenzentrum of the Max Planck Society, and on Compute Canada resources via project cfz-411-aa. +G. Allen acknowledges that this material is based upon work supported while +serving at the National Science Foundation. Any opinion, findings, and +conclusions or recommendations expressed in this material are those of the +authors and do not necessarily reflect the views of the National Science +Foundation. + \section*{References} \bibliographystyle{iopart-num-edit}

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 223)
by cott＠tapir.caltech.edu 14 Nov '11

14 Nov '11

User: cott Date: 2011/11/14 10:29 AM Modified: / ET.tex Log: * tiny File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +1 -1 =================================================================== --- ET.tex 2011-11-14 16:28:41 UTC (rev 222) +++ ET.tex 2011-11-14 16:29:10 UTC (rev 223) @@ -2923,7 +2923,7 @@ are expected to be running on 100,000 and more compute cores. \section*{Acknowledgments} -\todo{All: Add!} The authors with to thank Ed Seidel whose +\todo{All: Add!} The authors wish to thank Ed Seidel whose inspiration and vision has driven work towards the Einstein Toolkit over the past 15 years. The Einstein Toolkit is directly supported by the National Science Foundation in the USA under the grant numbers

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 222)
by cott＠tapir.caltech.edu 14 Nov '11

14 Nov '11

User: cott Date: 2011/11/14 10:28 AM Modified: / ET.tex Log: * tiny File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +13 -13 =================================================================== --- ET.tex 2011-11-14 16:28:10 UTC (rev 221) +++ ET.tex 2011-11-14 16:28:41 UTC (rev 222) @@ -2923,19 +2923,19 @@ are expected to be running on 100,000 and more compute cores. \section*{Acknowledgments} -\todo{All: Add!} -The authors with to thank Ed Seidel whose inspiration and vision has driven -work towards the Einstein Toolkit over the past 15 years. -The Einstein Toolkit is directly supported by the National Science -Foundation in the USA under the grant numbers 0903973/0903782/0904015 -(CIGR\@). Related grants contribute directly and indirectly to the -success of CIGR, including NSF OCI-0721915, NSF OCI-0725070, NSF -OCI-0832606, NSF OCI-0905046, NSF OCI-0941653, NSF AST-0855535, NSF -DMS-0820923, NASA 08-ATFP08-0093, EC-FP7 PIRG05-GA-2009-249290 and DFG -grant SFB/Transregio~7 ``Gravitational-Wave Astronomy''. Results -presented in this article were obtained through computations on the -Louisiana Optical Network Initiative under allocation loni\_cactus05 -and loni\_numrel07, as well as on NSF XSEDE under allocations +\todo{All: Add!} The authors with to thank Ed Seidel whose +inspiration and vision has driven work towards the Einstein Toolkit +over the past 15 years. The Einstein Toolkit is directly supported by +the National Science Foundation in the USA under the grant numbers +0903973/0903782/0904015 (CIGR\@). Related grants contribute directly +and indirectly to the success of CIGR, including NSF OCI-0721915, NSF +OCI-0725070, NSF OCI-0832606, NSF OCI-0905046, NSF OCI-0941653, NSF +AST-0855535, NSF DMS-0820923, NASA 08-ATFP08-0093, EC-FP7 +PIRG05-GA-2009-249290 and Deutsche Forschungsgemeinschaft grant +SFB/Transregio~7 ``Gravitational-Wave Astronomy''. Results presented +in this article were obtained through computations on the Louisiana +Optical Network Initiative under allocation loni\_cactus05 and +loni\_numrel07, as well as on NSF XSEDE under allocations TG-MCA02N014, TG-PHY060027N, TG-PHY100033, at the National Energy Research Scientific Computing Center (NERSC), which is supported by the Office of Science of the US Department of Energy under contract

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 221)
by cott＠tapir.caltech.edu 14 Nov '11

14 Nov '11

User: cott Date: 2011/11/14 10:28 AM Modified: / ET.tex Log: * tiny File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +1 -1 =================================================================== --- ET.tex 2011-11-14 16:27:37 UTC (rev 220) +++ ET.tex 2011-11-14 16:28:10 UTC (rev 221) @@ -2924,7 +2924,7 @@ \section*{Acknowledgments} \todo{All: Add!} -We wish to thank Ed Seidel whose inspiration and vision has driven +The authors with to thank Ed Seidel whose inspiration and vision has driven work towards the Einstein Toolkit over the past 15 years. The Einstein Toolkit is directly supported by the National Science Foundation in the USA under the grant numbers 0903973/0903782/0904015

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 220)
by cott＠tapir.caltech.edu 14 Nov '11

14 Nov '11

User: cott Date: 2011/11/14 10:27 AM Modified: / ET.tex Log: * add acknowledgement to Ed File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +10 -8 =================================================================== --- ET.tex 2011-11-14 16:04:04 UTC (rev 219) +++ ET.tex 2011-11-14 16:27:37 UTC (rev 220) @@ -2924,14 +2924,16 @@ \section*{Acknowledgments} \todo{All: Add!} -The Einstein Toolkit is directly supported by the -National Science Foundation in the USA under the grant numbers -0903973/0903782/0904015 (CIGR\@). Related grants contribute directly -and indirectly to the success of CIGR, including NSF OCI-0721915, NSF -OCI-0725070, NSF OCI-0832606, NSF OCI-0905046, NSF OCI-0941653, -NSF AST-0855535, NSF DMS-0820923, NASA 08-ATFP08-0093, EC-FP7 PIRG05-GA-2009-249290 and -DFG grant SFB/Transregio~7 ``Gravitational-Wave Astronomy''. -Results presented in this article were obtained through computations on the +We wish to thank Ed Seidel whose inspiration and vision has driven +work towards the Einstein Toolkit over the past 15 years. +The Einstein Toolkit is directly supported by the National Science +Foundation in the USA under the grant numbers 0903973/0903782/0904015 +(CIGR\@). Related grants contribute directly and indirectly to the +success of CIGR, including NSF OCI-0721915, NSF OCI-0725070, NSF +OCI-0832606, NSF OCI-0905046, NSF OCI-0941653, NSF AST-0855535, NSF +DMS-0820923, NASA 08-ATFP08-0093, EC-FP7 PIRG05-GA-2009-249290 and DFG +grant SFB/Transregio~7 ``Gravitational-Wave Astronomy''. Results +presented in this article were obtained through computations on the Louisiana Optical Network Initiative under allocation loni\_cactus05 and loni\_numrel07, as well as on NSF XSEDE under allocations TG-MCA02N014, TG-PHY060027N, TG-PHY100033, at the National Energy

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[svn:einsteintoolkit] manifest/trunk/ (Rev. 131)
by roland.haas＠physics.gatech.edu 14 Nov '11

14 Nov '11

User: rhaas Date: 2011/11/14 10:12 AM Modified: /trunk/ einsteintoolkit.bib Log: einsteintoolkit.bib: add arXiv:1009.0292 File Changes: Directory: /trunk/ ================== File [modified]: einsteintoolkit.bib Delta lines: +15 -0 =================================================================== --- trunk/einsteintoolkit.bib 2011-11-14 15:52:38 UTC (rev 130) +++ trunk/einsteintoolkit.bib 2011-11-14 16:12:37 UTC (rev 131) @@ -1773,6 +1773,21 @@ primaryClass = "gr-qc", } +@Article{Lousto:2010ut, + author = "Lousto, Carlos O. and Zlochower, Yosef", + title = "{Orbital Evolution of Extreme-Mass-Ratio Black-Hole + Binaries with Numerical Relativity}", + journal = "Phys. Rev. Lett.", + volume = "106", + year = "2011", + pages = "041101", + eprint = "1009.0292", + archivePrefix = "arXiv", + primaryClass = "gr-qc", + doi = "10.1103/PhysRevLett.106.041101", + SLACcitation = "%%CITATION = 1009.0292;%%" +} + ##M ############################################################################ @article{Manca:2007ca,

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 219)
by knarf＠cct.lsu.edu 14 Nov '11

14 Nov '11

User: knarf Date: 2011/11/14 10:04 AM Modified: / ET.tex Log: remove todo, for now File Changes: Directory: / ============ File [modified]: ET.tex Delta lines: +0 -1 =================================================================== --- ET.tex 2011-11-14 15:57:11 UTC (rev 218) +++ ET.tex 2011-11-14 16:04:04 UTC (rev 219) @@ -473,7 +473,6 @@ {\tt Carpet} is the main driver used today for {\tt Cactus}-based astrophysical simulations. {\tt Carpet} offers hybrid MPI/OpenMP parallelization and is used in production on up to several thousand cores~\cite{Reisswig:2010cd,Lousto:2010ut}. -\todo{if you use many cores in your runs: please speak up} \begin{figure} \centering \includegraphics[width=0.85\textwidth]{cactus-benchmarks/results-best}

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[svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 218)
by knarf＠cct.lsu.edu 14 Nov '11

14 Nov '11

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

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