[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 274)

[jfaber at einsteintoolkit.org]

User: jfaber
Date: 2012/03/09 10:29 AM

Modified:
 /
  ET.tex

Log:
 Fixed a few reference keys

File Changes:

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

File [modified]: ET.tex
Delta lines: +5 -5
===================================================================
--- ET.tex	2012-03-09 16:20:05 UTC (rev 273)
+++ ET.tex	2012-03-09 16:29:56 UTC (rev 274)
@@ -209,7 +209,7 @@
 on fixed background spacetimes has been successful in multi-dimensional
 settings since the mid-1990s, focusing on BH accretion processes and 
 relativistic jet production and evolution
-(see~\cite{Font:2008aa} for a review of the numerical formalism
+(see~\cite{Font:2007zz} for a review of the numerical formalism
 and~\cite{Hawley2009apss} for a review of work on disk and jet models). 
 GRMHD coupled with
 curvature evolution, on the other hand, which is crucial for modeling large-scale bulk
@@ -217,7 +217,7 @@
 started to produce astrophysically interesting results only in the
 past $\sim 3-5$ years, enabled primarily by the availability of long-term
 stable curvature evolution systems as well as improved GRMHD
-algorithms~(see~\cite{Font:2008aa} for a review). 
+algorithms~(see~\cite{Font:2007zz} for a review). 
 In addition to these developments, substantial progress has been made 
 in importing more physically motivated equations of state (EOS), 
 including tabulated versions (e.g.,~\cite{Pandharipande:1989hn,
@@ -837,7 +837,7 @@
 
 \codename{HydroBase} uses a set of conventions known as the Valencia
 formulation~\cite{Marti:1991wi,Banyuls:1997zz,Ibanez:2001:godunov}.
-In particular, \codename{HydroBase} defines the primitive variables (see~\cite{Font:2008aa} for
+In particular, \codename{HydroBase} defines the primitive variables (see~\cite{Font:2007zz} for
 details):
 \begin{itemize}
  \item \verb|rho|: rest mass density $\rho$
@@ -3054,8 +3054,8 @@
 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:2010ze,Reisswig:2010cd,Reisswig:2009rx}.  The authors of one such
+CCE code~\cite{Babiuc:2010ze} have agreed to make their work available to the
 whole community by integrating their CCE routines into the Einstein Toolkit
 release 2011\_11 ``Maxwell,'' which will be described elsewhere.