diff options
author | rhaas <rhaas@1bdb13ef-5d69-4035-bb54-08abeb3aa7f1> | 2013-07-08 06:45:43 +0000 |
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committer | rhaas <rhaas@1bdb13ef-5d69-4035-bb54-08abeb3aa7f1> | 2013-07-08 06:45:43 +0000 |
commit | 7337d16bc3e4866f5011dd5a88ea76fb3c5f29da (patch) | |
tree | cefff6c089825423ae0f58966de784959c64c69e /src | |
parent | f1e06328a789a6c203ae9043258cc815b0e047ef (diff) |
remove duplicate parameter from test_two_max test
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/TOVSolver/trunk@140 1bdb13ef-5d69-4035-bb54-08abeb3aa7f1
Diffstat (limited to 'src')
-rw-r--r-- | src/tov.c | 13 |
1 files changed, 7 insertions, 6 deletions
@@ -844,20 +844,21 @@ void TOV_C_Exact(CCTK_ARGUMENTS) /* It is absolutely idiotic to have different atmosphere thresholds for different stars that are placed on the same goddamn grid. This also screws symmetry, so - we get rid of it /* - /* if(rho[i3D] <= TOV_Atmosphere[star_i]) { + we get rid of it \* + \* */ if(rho[i3D] <= TOV_Atmosphere[star_i]) { rho[i3D] = TOV_Atmosphere[star_i]; - press[i3D] = TOV_K[star_i] * pow(rho[i3D],TOV_Gamma[star_i]); - eps[i3D] = press[i3D]/(TOV_Gamma[star_i]-1.0)/rho[i3D]; - } */ + press[i3D] = TOV_K * pow(rho[i3D],TOV_Gamma); + eps[i3D] = press[i3D]/(TOV_Gamma-1.0)/rho[i3D]; + } /**/ } - +#if 0 if(rho[i3D] <= TOV_Atmosphere[0]) { rho[i3D] = TOV_Atmosphere[0]; press[i3D] = TOV_K * pow(rho[i3D],TOV_Gamma); eps[i3D] = press[i3D]/(TOV_Gamma-1.0)/rho[i3D]; } +#endif if (TOV_Conformal_Flat_Three_Metric) { |