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author | rhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45> | 2011-09-15 16:42:47 +0000 |
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committer | rhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45> | 2011-09-15 16:42:47 +0000 |
commit | 3fe900e7b6808a214b3341bf923bd57a67ce9450 (patch) | |
tree | 54c3c92a17618328e021c2b9b21d27c2f9116c9a /param.ccl | |
parent | 52ed503635a6c5dc06bd8bd8866b6eb6f00ec28b (diff) |
add option to smoothly dampen Tmunu to vacuum outside of a given radius
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@266 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
Diffstat (limited to 'param.ccl')
-rw-r--r-- | param.ccl | 16 |
1 files changed, 16 insertions, 0 deletions
@@ -532,6 +532,22 @@ boolean track_divB "Track the magnetic field constraint violations" { } "no" +############### Parameters for Tmunu damping (useful in atmosphere) ##################### + +CCTK_REAL Tmunu_damping_radius_min "damping radius at which we start to damp with a tanh function" +{ + -1 :: "damping switched off" + 0:* :: "damping radius at which we start to damp" +} -1 + + +CCTK_REAL Tmunu_damping_radius_max "damping radius at which Tmunu becomes 0" +{ + -1 :: "damping switched off" + 0:* :: "greater than minimum radius above" +} -1 + + ############### temporary parameters to be removed once connected issues are fixed. boolean con2prim_oct_hack "Disregard c2p failures in oct/rotsym90 boundary cells with xyz < 0" STEERABLE=ALWAYS |