[Commits] [svn:einsteintoolkit] Paper_EinsteinToolkit_2010/ (Rev. 98)

[knarf at cct.lsu.edu]

User: knarf
Date: 2011/08/01 11:06 AM

Modified:
 /
  ET.tex

Log:
 get some of the structure of the evolution methods straight

File Changes:

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

File [modified]: ET.tex
Delta lines: +5 -6
===================================================================
--- ET.tex	2011-08-01 15:50:41 UTC (rev 97)
+++ ET.tex	2011-08-01 16:05:59 UTC (rev 98)
@@ -966,9 +966,8 @@
 one may also apply a uniform velocity to the neutron star, though this does not affect 
 the ODE solution nor the resulting density profile.
 
-\subsection{Spacetime Curvature Evolution}
+\subsection{Spacetime Curvature Evolution}\todo{Peter: move}
 \label{sec:evol}
-\todo{Josh and Christian in charge}
 
 In the following, we assume that the reader is familiar with the
 basics of numerical relativity and GR hydrodynamics. Detailed
@@ -1004,7 +1003,7 @@
 the relativistic specific enthalpy with $\epsilon$ and $P$ being the
 specific internal energy and the pressure, respectively.
 
-\subsubsection{Spacetime Curvature Evolution}
+\subsection{Spacetime Curvature Evolution}
 \label{sec:Kevol}
 The Einstein Toolkit
 curvature evolution code \codename{McLachlan}~\cite{brown:09,reisswig:11ccwave} is
@@ -1173,7 +1172,7 @@
 
 
 
-\paragraph{Initial Conditions}
+\subsubsection{Initial Conditions}
 
 Initial conditions from the ADM variables $g_{ij}$, $K_{ij}$, lapse
 $\alpha$, and shift $\beta^i$, as provided by the initial data
@@ -1197,7 +1196,7 @@
 then defined via the points in the interior and the previously
 calculated layers.
 
-\paragraph{Boundary Conditions}
+\subsubsection{Boundary Conditions}
 \label{sec:curv_boundaries}
 
 During time evolution, a Sommerfeld-type radiative boundary condition
@@ -1266,7 +1265,7 @@
  gauge conditions used in \codename{McLachlan}.
 
 
-\subsection{Hydrodynamics: \codename{GRHydro}}\pages{Christian and Josh}
+\subsection{Hydrodynamics Evolution}\pages{Christian and Josh}
 \label{sec:GRHydro}
 
 {\color{red} This text is copied from Reisswig et al. It needs to be expanded a bit and we probably want to talk about the numerical methods a bit more.}