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| author | schnetter <schnetter@c3c03602-0f4f-0410-b3fa-d2c81c8a7dc5> | 2009-02-10 22:26:07 +0000 |
|---|---|---|
| committer | schnetter <schnetter@c3c03602-0f4f-0410-b3fa-d2c81c8a7dc5> | 2009-02-10 22:26:07 +0000 |
| commit | ef578b0e0a60a99f3c78781088f586ba3eac3b4b (patch) | |
| tree | 660ae5413c6c4b49f365f16aee93b8ebb784ec19 /README | |
| parent | 82f03c37bc8659c8134b1a0d2e8d06963bc2633c (diff) | |
Update README and licence.
git-svn-id: http://svn.cactuscode.org/arrangements/CactusNumerical/RotatingSymmetry90/trunk@45 c3c03602-0f4f-0410-b3fa-d2c81c8a7dc5
Diffstat (limited to 'README')
| -rw-r--r-- | README | 11 |
1 files changed, 5 insertions, 6 deletions
@@ -1,14 +1,13 @@ -CVS info : $Header$ - Cactus Code Thorn RotatingSymmetry90 -Thorn Author(s) : Erik Schnetter <schnetter@aei.mpg.de> -Thorn Maintainer(s) : Erik Schnetter <schnetter@aei.mpg.de> +Author(s) : Erik Schnetter <schnetter@cct.lsu.edu> +Maintainer(s): Erik Schnetter <schnetter@cct.lsu.edu> +Licence : GPL -------------------------------------------------------------------------- -Purpose of the thorn: +1. Purpose Provide a 90 degree rotational symmetry boundary condition. This is -the kind of symmetry that exists e.g. in a singl black hole evolution +the kind of symmetry that exists e.g. in a single black hole evolution when the black hole has spin. The same setup also admits an additional bitant symmetry. |