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authorknarf <knarf@6a3ddf76-46e1-4315-99d9-bc56cac1ef84>2010-10-07 16:42:08 +0000
committerknarf <knarf@6a3ddf76-46e1-4315-99d9-bc56cac1ef84>2010-10-07 16:42:08 +0000
commit8b1c7440296e61926ce950995b6d7c2b8e9e49fb (patch)
tree49db6fee5c071c2f32c51980f59d6a625c4ac2c5 /src
parent67d93eee204f939ad97713873efcdac5fc9eb8db (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 'src')
-rw-r--r--src/Kerr.c2
1 files changed, 1 insertions, 1 deletions
diff --git a/src/Kerr.c b/src/Kerr.c
index ae39fd6..d7966ca 100644
--- a/src/Kerr.c
+++ b/src/Kerr.c
@@ -132,7 +132,7 @@ void KerrID(CCTK_ARGUMENTS)
p2=a_2+r_2-a*beta_phi;
/* drdR=sqrt_Delta/R; */
lapse=sqrt_Delta/sqrt(p2);
- shift_phi=-2*m*rK*a/p2;
+ shift_phi=-2*m*rK*a/(p2*Sigma);
/* Kerr metric in quasi-isotropic coordinates */
/* ds^2=Phi4*(dR^2+R^2*dth^2+R^2*Chi^2*sin(th)^2*dphi^2) */