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author | jthorn <jthorn@0a4070d5-58f5-498f-b6c0-2693e757fa0f> | 2006-07-17 15:05:29 +0000 |
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committer | jthorn <jthorn@0a4070d5-58f5-498f-b6c0-2693e757fa0f> | 2006-07-17 15:05:29 +0000 |
commit | 25a07bedeb52fd50058d79b05ac19ae79e8c4beb (patch) | |
tree | c955dac6cca1d3ce3480496510d8f1e7a4932b0d | |
parent | 54576d0949701ee14ad024b6d2dae3e6e1d6d1b4 (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
-rw-r--r-- | doc/documentation.tex | 16 |
1 files changed, 16 insertions, 0 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex index 5cb2fff..0c4bec3 100644 --- a/doc/documentation.tex +++ b/doc/documentation.tex @@ -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 |