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author | eschnett <eschnett@4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843> | 2010-03-29 10:45:17 +0000 |
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committer | eschnett <eschnett@4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843> | 2010-03-29 10:45:17 +0000 |
commit | f33a18fee7267ff212baec75795ecb13670643e8 (patch) | |
tree | 26461682ee96a7bd5f8da6879432d88fe49e2124 /README | |
parent | d7ddbe354ebe7072ff6687124e5f620d56a16b28 (diff) |
Make self-updating work again after moving the "m" directory into the
thorn.
Add README.
Re-generate thorn.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/WeylScal4/trunk@51 4f5cb9a8-4dd8-4c2d-9bbd-173fa4467843
Diffstat (limited to 'README')
-rw-r--r-- | README | 18 |
1 files changed, 18 insertions, 0 deletions
@@ -0,0 +1,18 @@ +Cactus Code Thorn WeylScal4 +Author(s) : Roland Haas + Erik Schnetter +Maintainer(s): Cactus team +Licence : LGPL +-------------------------------------------------------------------------- + +1. Purpose + +Calculate the Weyl Scalars for a given metric. + + + +2. Implementation + +The code is generated automatically with Mathematica. The Mathematica +scripts are in the subdirectory "m", and the Makefile in there +re-generates the code. This requires Mathematica to be installed. |