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authorikelley <ikelley@0a4070d5-58f5-498f-b6c0-2693e757fa0f>2002-06-04 12:50:57 +0000
committerikelley <ikelley@0a4070d5-58f5-498f-b6c0-2693e757fa0f>2002-06-04 12:50:57 +0000
commitca3964cfed918b8c0956a68ce4fd4c4393cab760 (patch)
treeaa941c67776d03d6edd138a378a9913e75a6dd8d
parent95e0ddb903da16f7cebfdf5a7757f21c1518b79d (diff)
changing the documentation.tex files to use our cactus style file
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAxiBrillBH/trunk@50 0a4070d5-58f5-498f-b6c0-2693e757fa0f
-rw-r--r--doc/documentation.tex23
1 files changed, 20 insertions, 3 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex
index 8567c19..a7350c5 100644
--- a/doc/documentation.tex
+++ b/doc/documentation.tex
@@ -1,16 +1,29 @@
\documentclass{article}
+
+% Use the Cactus ThornGuide style file
+% (Automatically used from Cactus distribution, if you have a
+% thorn without the Cactus Flesh download this from the Cactus
+% homepage at www.cactuscode.org)
+\usepackage{../../../../doc/ThornGuide/cactus}
+
\begin{document}
\title{IDAxiBrillBH}
\author{Paul Walker, Steve Brandt}
-\date{1 September 1999}
+\date{$ $Date$ $}
+
\maketitle
-\abstract{Thorn IDAxiBrillBH provides analytic initial data for a vacuum
+% Do not delete next line
+% START CACTUS THORNGUIDE
+
+\begin{abstract}
+ Thorn IDAxiBrillBH provides analytic initial data for a vacuum
black hole spacetime: a single Schwarzschild black hole in
isotropic coordinates plus Brill wave. This initial data is
provided for the 3-conformal metric, it's spatial derivatives, and
- extrinsic curvature.}
+ extrinsic curvature.
+\end{abstract}
\section{Purpose}
@@ -158,4 +171,8 @@ interpolation.
\bibitem{Camarda97a}
K. Camarda, Ph.D thesis University of Illinois Urbana-Champaign, (1998)
\end{thebibliography}
+
+% Do not delete next line
+% END CACTUS THORNGUIDE
+
\end{document}