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author | knarf <knarf@6a3ddf76-46e1-4315-99d9-bc56cac1ef84> | 2010-10-07 16:42:08 +0000 |
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committer | knarf <knarf@6a3ddf76-46e1-4315-99d9-bc56cac1ef84> | 2010-10-07 16:42:08 +0000 |
commit | 8b1c7440296e61926ce950995b6d7c2b8e9e49fb (patch) | |
tree | 49db6fee5c071c2f32c51980f59d6a625c4ac2c5 /doc/documentation.tex | |
parent | 67d93eee204f939ad97713873efcdac5fc9eb8db (diff) |
correct computation of shift vector in Kerr metric, along with the documentation and a proof that this is right
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/IDAnalyticBH/trunk@175 6a3ddf76-46e1-4315-99d9-bc56cac1ef84
Diffstat (limited to 'doc/documentation.tex')
-rw-r--r-- | doc/documentation.tex | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/doc/documentation.tex b/doc/documentation.tex index 0de53c7..45727f0 100644 --- a/doc/documentation.tex +++ b/doc/documentation.tex @@ -194,7 +194,7 @@ The gauge can be set to the Kerr lapse and shift with the parameters in which case the formulas \begin{eqnarray} \alpha & = &\sqrt{\frac{\Delta}{p^2}}, \\ - \beta^\phi & = & -2 m r_k a / p^2, + \beta^\phi & = & -2 m r_k a / (p^2 \Sigma), \end{eqnarray} where \begin{equation} |