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