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.
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