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author | rhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45> | 2013-01-14 14:23:23 +0000 |
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committer | rhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45> | 2013-01-14 14:23:23 +0000 |
commit | e6697d32350c5dab48bf59d2b36989e3ef15f21e (patch) | |
tree | 01f336b3978ddb3ccaa800f16250f77d59c00467 /param.ccl | |
parent | 4284e5495d1162cf347be5bd109ee6d271d46179 (diff) |
GRHydro: call polytrope EOS in a region dominated by mag. field.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@451 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
Diffstat (limited to 'param.ccl')
-rw-r--r-- | param.ccl | 5 |
1 files changed, 5 insertions, 0 deletions
@@ -356,6 +356,11 @@ REAL sqrtdet_thr "Threshold to apply cons rescalings deep inside the horizon" ST 1.0: :: "Larger values guarantees this sort of rescaling only deep inside the horizon" } 30.0 +REAL max_magnetic_to_gas_pressure_ratio "consider pressure to be magnetically dominated if magnetic pressure to gas pressure ratio is higher than this" STEERABLE=ALWAYS +{ + (0:* :: "any positive value, eg. 100." + -1.0 :: "disable" +} -1.0 boolean c2p_reset_pressure "If the pressure guess is unphysical should we recompute it?" { |