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-\documentstyle{report}
-\newcommand{\parameter}[1]{{\it #1}}
-
-\begin{document}
-
-\chapter{IDAnalyticBH}
-
-\begin{tabular}{@{}ll}
-Code Authors & Joan Masso, Paul Walker, Ed Seidel. Gabrielle Allen \\
-Maintained by & Cactus Developers \\
-Documentation Authors & 
-\end{tabular}
-
-\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{Extended Parameters}
-\begin{tabular}{l|l|l|l}
-&&&\\
-einstein &&&\\
-\hline
-\parameter{initial\_data} & KEYWORD & schwarzschild & One Schwarzschild black hole \\
-& & bl\_bh & Brill Lindquist black holes \\
-& & misner\_bh &Misner black holes \\
-& & multiple\_misner\_bh & Multiple Misner black holes \\
-\parameter{initial\_lapse} & KEYWORD & schwarz & Set lapse to schwarzschild \\
-\end{tabular}
-
-\subsection{Private Parameters}
-
-\begin{tabular}{l|l|l|l|l}
-&&&&\\
-Schwarzschild & & & & \\
-\hline
-\parameter{mass} & {\t CCTK\_REAL} & $(-\infty,\infty)$ & 2.0 & Mass of black hole \\
-&&&&\\
-Multiple Misner & & & & \\
-\hline
-\parameter{mu} & {\t CCTK\_REAL} & $[0,\infty)$ & 1.2 & Misner $\mu$ value \\
-\parameter{nmax} & {\t CCTK\_INT} & $[0,\infty)$ & 30 & Numer of terns to include for Misner series \\
-\parameter{misner\_nmh} & {\t CCTK\_INT} & $[0,10]$ & 1 & Number of Misner black holes \\
-&&&&\\
-Brill Lindquist & & & & \\
-\hline
-\parameter{bl\_nbh} & {\t CCTK\_INT} & $[1,4]$ & 1 & Number of Brill Lindquist black holes\\
-\parameter{bl\_x0\_1} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 & x-position of first BL hole\\
-\parameter{bl\_y0\_1} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  y-position of first BL hole\\
-\parameter{bl\_z0\_1} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  z-position of first BL hole\\
-\parameter{bl\_M\_1} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 1.0 &  mass of first BL hole\\
-\parameter{bl\_x0\_2} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 & x-position of second BL hole\\
-\parameter{bl\_y0\_2} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  y-position of second BL hole\\
-\parameter{bl\_z0\_2} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  z-position of second BL hole\\
-\parameter{bl\_M\_2} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 1.0 &  mass of second BL hole\\
-\parameter{bl\_x0\_3} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 & x-position of third BL hole\\
-\parameter{bl\_y0\_3} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  y-position of third BL hole\\
-\parameter{bl\_z0\_3} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  z-position of third BL hole\\
-\parameter{bl\_M\_3} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 1.0 &  mass of third BL hole\\
-\parameter{bl\_x0\_4} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 & x-position of fourth BL hole\\
-\parameter{bl\_y0\_4} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  y-position of fourth BL hole\\
-\parameter{bl\_z0\_4} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 0.0 &  z-position of fourth BL hole\\
-\parameter{bl\_M\_4} & {\t CCTK\_REAL} &  $(-\infty,\infty)$ & 1.0 &  mass of fourth BL hole\\
-\end{tabular}
-
-\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}