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authorallen <allen@6a3ddf76-46e1-4315-99d9-bc56cac1ef84>1999-04-01 18:10:24 +0000
committerallen <allen@6a3ddf76-46e1-4315-99d9-bc56cac1ef84>1999-04-01 18:10:24 +0000
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tree5dc674bd5fe7f5c29cd516676988531c7402de34 /doc
parent2e3b8edde7db995fe5f2f66aec79b2fdb86e94e1 (diff)
This is going to be an example of how to write thorn documentation, at
the moment it is an example of how not to write thorn documentation git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAnalyticBH/trunk@13 6a3ddf76-46e1-4315-99d9-bc56cac1ef84
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+\documentstyle{report}
+%\def{\parameter{#1}}{{\it #1}}
+
+\begin{document}
+
+\chapter{IDAnalyticBH}
+
+\section{Introduction}
+
+\subsection{Purpose of Thorn}
+
+Thorn IDAnalyticBH provides analytic initial data for vacuum black
+hole spacetimes. Initial data is provided for the 3-metric, extrinsic
+curvature, and if appropriate the conformal factor and it's spatial
+derivatives. The current initial data sets are for a single (Schwarzschild)
+black hole in isotropic coordinates, up to four Brill-Lindquist black
+holes, and any number of Misner-type black holes.
+
+\subsection{Technical Specification}
+
+\begin{itemize}
+
+\item{Implements} einsteinID
+\item{Inherits from} einstein
+\item{Tested with thorns} Einstein
+
+\end{itemize}
+
+\section{Theoretical Background}
+
+
+\section{Algorithmic and Implementation Details}
+
+This thorn uses no special numerical methods, however two points
+are worth noting
+
+\begin{enumerate}
+
+\item{} The solution for Misner is obtained by summing a sequence
+
+\item{} The spatial derivatives of the conformal metric (when required)
+ are calculated accurately using finite differencing of the
+ exact solution by a very small spacing
+
+\end{enumerate}
+
+\section{Using the Thorn}
+
+This thorn can provide either the physical metric (use\_conformal=''no'')
+or the conformal metric and a conformal factor (and its spatial derivatives)
+(use\_conformal=''yes''). In general, the option use\_conformal=''yes'' should
+be used, since ????.
+
+\section{Parameters}
+
+\subsection{List of all Parameters}
+
+\subsection{Discussion}
+
+\section{Interaction with Other Thorns}
+
+It is still to be decided how initial data should be supplied to
+for systems of evolution equations which use more or different
+variables to those in the einstein implementation
+
+\section{Future Development}
+
+Initial data sets which are missing from this thorn include
+
+\begin{itemize}
+
+\item{} Boosted single black hole
+\item{} Single black hole in harmonic spatial coordinates
+\item{} Single black hole in Eddington-Finkelstein coordinates
+
+\end{itemize}
+
+
+\end{document}