[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 208)

[knarf at cct.lsu.edu]

User: knarf
Date: 2011/11/14 02:39 AM

Modified:
 /
  ET.tex

Log:
 cosmetics in future work section

File Changes:

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

File [modified]: ET.tex
Delta lines: +3 -3
===================================================================
--- ET.tex	2011-11-14 08:35:47 UTC (rev 207)
+++ ET.tex	2011-11-14 08:39:49 UTC (rev 208)
@@ -2881,8 +2881,8 @@
 improvement. One example is the need for the gauge invariant
 extraction of gravitational waves from simulation spacetimes as realized
 by the Cauchy Characteristic Extraction (CCE) technique recently studied
-in \cite{Babiuc:11,Reisswig:2010cd,Reisswig:2011a}.  The authors of one such
-CCE code \cite{Babiuc:11} have agreed to make their work available to the
+in~\cite{Babiuc:11,Reisswig:2010cd,Reisswig:2011a}.  The authors of one such
+CCE code~\cite{Babiuc:11} have agreed to make their work available to the
 whole community by integrating their CCE routines into the Einstein Tookit
 release 2011\_11 ``Maxwell,'' which will be described elsewhere.
 
@@ -2928,7 +2928,7 @@
   Carpet} AMR infrastructure. As we have shown, good scaling is
 limited to only a few thousand processes for some of the most widely used
 simulation scenarios.  Work is in progress to eliminate this
-bottle-neck.  On the other hand, a production simulation is typically
+bottleneck.  On the other hand, a production simulation is typically
 composed of a large number of components, and even analysis and I/O
 routines have to scale well to achieve overall good performance. This
 is a highly non-trivial problem, since most Einstein Toolkit physics