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

Modified: / ET.tex

Log: Remove todo

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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