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author | diener <diener@2a26948c-0e4f-0410-aee8-f1d3e353619c> | 2002-04-11 12:45:53 +0000 |
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committer | diener <diener@2a26948c-0e4f-0410-aee8-f1d3e353619c> | 2002-04-11 12:45:53 +0000 |
commit | c049541c04620a927261fe2bed99654fdccee0e6 (patch) | |
tree | 70071897d45f073e02ddda0e5d5f590814def2ce /README | |
parent | c222203c5ac0fd628ba23be2c31be883de4755c7 (diff) |
Initial files for the event horizon thorn. Everything is still empty.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/EHFinder/trunk@2 2a26948c-0e4f-0410-aee8-f1d3e353619c
Diffstat (limited to 'README')
-rw-r--r-- | README | 14 |
1 files changed, 14 insertions, 0 deletions
@@ -0,0 +1,14 @@ +Cactus Code Thorn EHFinder +Authors : Peter Diener +CVS info : $Header$ +-------------------------------------------------------------------------- + +Purpose of the thorn: + +To find the event horizon of a numerical spacetime by integrating a null +surface backwards in time. The basic equation is equation 2 in Anninos et. al, +Physical Review Letters, 74, 630, 1995. + +The surface will be parametrized as the 0 value isosurface of a level +set function. Hopefully this will work when the topology changes from +one common event horizon to two individual event horizons. |