diff options
| author | cott <cott@1bdb13ef-5d69-4035-bb54-08abeb3aa7f1> | 2013-07-07 05:34:05 +0000 |
|---|---|---|
| committer | cott <cott@1bdb13ef-5d69-4035-bb54-08abeb3aa7f1> | 2013-07-07 05:34:05 +0000 |
| commit | ea70d0ee2becfeabce8fbc261779c571da1572e0 (patch) | |
| tree | 59c33ed64b2337d29e9f75692b26001e6ba9a704 /test/test_two_av.par | |
| parent | 3428e526a579605f5db67ee2ce29694f4dcc88f4 (diff) | |
* remove option to have different gamma and K for different
stars. That's physically impossible.
* adjust test par files (will do so with GRHydro next)
* modify the way solutions are added so that atmosphere cuts
are applied after solutions are added. Otherwise one of the
stars will have the atmosphere added to it. This breaks symmetry.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/TOVSolver/trunk@137 1bdb13ef-5d69-4035-bb54-08abeb3aa7f1
Diffstat (limited to 'test/test_two_av.par')
| -rw-r--r-- | test/test_two_av.par | 8 |
1 files changed, 4 insertions, 4 deletions
diff --git a/test/test_two_av.par b/test/test_two_av.par index 0b5725e..8f074b0 100644 --- a/test/test_two_av.par +++ b/test/test_two_av.par @@ -45,13 +45,13 @@ tovsolver::TOV_Num_Radial = 200000 tovsolver::TOV_Combine_Method = "average" tovsolver::TOV_Rho_Central[0] = 0.16e-3 -tovsolver::TOV_Gamma[0] = 2.0 -tovsolver::TOV_K[0] = 100.0 +tovsolver::TOV_Gamma = 2.0 +tovsolver::TOV_K = 100.0 tovsolver::TOV_Position_x[0] = -15.0 tovsolver::TOV_Rho_Central[1] = 0.32e-3 -tovsolver::TOV_Gamma[1] = 2.0 -tovsolver::TOV_K[1] = 100.0 +tovsolver::TOV_Gamma = 2.0 +tovsolver::TOV_K = 100.0 tovsolver::TOV_Position_x[1] = 15.0 IO::out_fileinfo="none" |