diff options
| author | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2002-10-22 19:54:26 +0000 |
|---|---|---|
| committer | jthorn <jthorn@f88db872-0e4f-0410-b76b-b9085cfa78c5> | 2002-10-22 19:54:26 +0000 |
| commit | 5f29e8d72162d4fe0a89bef240f855d81d8d5239 (patch) | |
| tree | 846e15f2a444806e312aad81ffdd99cd47c2e091 /doc | |
| parent | 0464ba379b188ea26accb87362a368e577f7fff6 (diff) | |
add:
handle quadrant/octant grids with symmetry BCs
(I think current Jacobian data structures can handle this,
I just need to define a new type of patch system)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/AHFinderDirect/trunk@852 f88db872-0e4f-0410-b76b-b9085cfa78c5
Diffstat (limited to 'doc')
| -rw-r--r-- | doc/TODO | 5 |
1 files changed, 4 insertions, 1 deletions
@@ -5,6 +5,9 @@ small things apparent horizon centroid, area, and mass medium things + handle quadrant/octant grids with symmetry BCs + (I think current Jacobian data structures can handle this, + I just need to define a new type of patch system) there should be a Cactus test suite HDF5 data files (simple format and/or Werner Benger's fancy one) move origin point to track moving BHs @@ -19,6 +22,6 @@ medium things large things multi-processor (interpolator, overall control) sparse matrix elliptic solver - handle quadrant/octant grids + handle quadrant/octant grids with rotating BCs (needs Jacobian of one ghost zone to cover two different ghost zones) "isolated horizons" computation of BH mass and spin |