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authorjthorn <jthorn@0a4070d5-58f5-498f-b6c0-2693e757fa0f>2006-07-17 15:05:29 +0000
committerjthorn <jthorn@0a4070d5-58f5-498f-b6c0-2693e757fa0f>2006-07-17 15:05:29 +0000
commit25a07bedeb52fd50058d79b05ac19ae79e8c4beb (patch)
treec955dac6cca1d3ce3480496510d8f1e7a4932b0d
parent54576d0949701ee14ad024b6d2dae3e6e1d6d1b4 (diff)
document normalization for the slice mass & AH radius
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAxiBrillBH/trunk@100 0a4070d5-58f5-498f-b6c0-2693e757fa0f
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@@ -152,6 +152,22 @@ and outer boundary condition, a Robin condition:
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\section{The Resulting Slice}
+
+This thorn normalizes things so that if there is no perturbation,
+it produces a Schwarzschild ($=$ Brill-Lindquist) slice of the $m=2$
+Schwarzschild spacetime.%%%
+\footnote{%%%
+ This slice has an apparent horizon at a
+ coordinate radius $r=1$.
+ }%%%
+{} You can't change this mass. :(
+
+In any case (perturbation or not), this thorn also reports an ADM mass
+for the slice. This seems to be pretty reliable.
+
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+
\section{2-D Grid and Interpolation Parameters}
This thorn solves equation~(\ref{IDAxiBrillBH/eqn:ham-linear}) on a 2-D