diff options
| author | pollney <pollney@6a3ddf76-46e1-4315-99d9-bc56cac1ef84> | 2002-06-10 07:35:57 +0000 |
|---|---|---|
| committer | pollney <pollney@6a3ddf76-46e1-4315-99d9-bc56cac1ef84> | 2002-06-10 07:35:57 +0000 |
| commit | c166fe1107292aed2fb056e5c10de9ddf18c3d06 (patch) | |
| tree | 35ebb6b95c57924920fb773ab6bf566cc632a40f | |
| parent | c6eee0bab612c5586d906090941d51efef5a2370 (diff) | |
Added explicit statement that Kerr assumes rotation about z-axis.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAnalyticBH/trunk@120 6a3ddf76-46e1-4315-99d9-bc56cac1ef84
| -rw-r--r-- | doc/documentation.tex | 3 |
1 files changed, 2 insertions, 1 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex index d9ea1f4..6bc4416 100644 --- a/doc/documentation.tex +++ b/doc/documentation.tex @@ -164,7 +164,8 @@ where \Sigma & = & {r_k}^2 + a^2 \cos^2\theta. \end{eqnarray} The two free parameters are the Kerr mass, $M$, and angular momentum, -$a$. These are specified using the parameters +$a$ (assumed to be aligned with the z-axis). +These are specified using the parameters \texttt{idanalyticbh::mass} and \texttt{idanalyticbh::a\_kerr} respectively. \emph{(Note that the default values for these parameters are $M=2$ and $a=0.1$.)} The black hole is assumed to reside at the |