[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 215)

[jfaber at einsteintoolkit.org]

User: jfaber
Date: 2011/11/14 09:43 AM

Modified:
 /
  ET.tex

Log:
 Added three references for 1990's cactus development, 2 typo fixes
 I have the bibfile ready for an update, missing refs will come shortly

File Changes:

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

File [modified]: ET.tex
Delta lines: +3 -3
===================================================================
--- ET.tex	2011-11-14 15:41:22 UTC (rev 214)
+++ ET.tex	2011-11-14 15:43:11 UTC (rev 215)
@@ -369,7 +369,7 @@
 an open source, modular, portable programming environment for
 collaborative HPC computing primarily developed at Louisiana State University,
 which originated at the Albert Einstein Institute and also has roots
-at the National Center for Supercomputing Applications.
+at the National Center for Supercomputing Applications~(see, e.g.,~\cite{Anninos:1995am,Anninos:1996ai,Seidel:1999ey} for historical reviews).
 The {\tt Cactus} computational toolkit consists of general modules which provide
 parallel drivers, coordinates, boundary conditions, interpolators,
 reduction operators, and efficient I/O in different data
@@ -2196,10 +2196,10 @@
 \section{Examples}
 \todo{Update if necessary}
 
-To demonstrate the properties of the code and its capabilities, we have used it to simulate common astrophysical configurations of interest.  Given the community-oriented direction of the project, the parameter files required to launch these simulations and a host of others are included and documented in the code releases, along with the datafiles produced by a representative set of simulation parameters to allow for code validation and confirmation of correct code performance on new platforms and architetures.  As part of the internal validation process, 
+To demonstrate the properties of the code and its capabilities, we have used it to simulate common astrophysical configurations of interest.  Given the community-oriented direction of the project, the parameter files required to launch these simulations and a host of others are included and documented in the code releases, along with the datafiles produced by a representative set of simulation parameters to allow for code validation and confirmation of correct code performance on new platforms and architectures.  As part of the internal validation process, 
 nightly builds are checked against a set of benchmarks to ensure that consistent results are generated with the inclusion of all new commits to the code.
 
-The performance of the Toolkit for vacuum configurations is demonstrated through evolutions of single, rotating BHs and the merger of binary black hole configurations (sections~\ref{sec:1bh-example} and \ref{sec:bbh-example}, respectively).   Linear oscillations about equilibirum for an isolated NS are discussed in section~\ref{sec:tov_oscillations}, and the collapse of a NS to a BH, including dynamical formation of a horizon, in section~\ref{sec:collapse_example}.  Finally, to show a less traditional application of the code, we show its ability to perform cosmological simulations by evolving a Kasner spacetime (see section~\ref{sec:cosmology}).
+The performance of the Toolkit for vacuum configurations is demonstrated through evolutions of single, rotating BHs and the merger of binary black hole configurations (sections~\ref{sec:1bh-example} and \ref{sec:bbh-example}, respectively).   Linear oscillations about equilibrium for an isolated NS are discussed in section~\ref{sec:tov_oscillations}, and the collapse of a NS to a BH, including dynamical formation of a horizon, in section~\ref{sec:collapse_example}.  Finally, to show a less traditional application of the code, we show its ability to perform cosmological simulations by evolving a Kasner spacetime (see section~\ref{sec:cosmology}).
 
 \subsection{Spinning BH}
 \label{sec:1bh-example}