[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 212)

[schnetter at cct.lsu.edu]

User: eschnett
Date: 2011/11/14 09:37 AM

Modified:
 /
  ET.tex

Log:
 Remove todo

File Changes:

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

File [modified]: ET.tex
Delta lines: +4 -1
===================================================================
--- ET.tex	2011-11-14 15:35:32 UTC (rev 211)
+++ ET.tex	2011-11-14 15:37:03 UTC (rev 212)
@@ -2548,7 +2548,10 @@
 The examples in the previous subsections did not include the evolution of
 matter within a relativistic spacetime. One interesting test of a coupled
 matter-spacetime evolution is to measure the eigenfrequencies of a stable TOV
-star~(see, e.g.,~\cite{Gourgoulhon:1991aa,Romero:1996aa,Shibata:1998sg,Font:2001ew,Shibata:2003iy}). \todo{Do we need more refs?  Five is decent for an e.g.}  These eigenfrequencies can be compared
+star~(see,
+e.g.,~\cite{Gourgoulhon:1991aa, Romero:1996aa, Shibata:1998sg,
+  Font:2001ew, Shibata:2003iy}).
+These eigenfrequencies can be compared
 to values known from linear perturbation theory.
 
 We begin our simulations with  a self-gravitating fluid