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authorrhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45>2011-09-15 16:42:47 +0000
committerrhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45>2011-09-15 16:42:47 +0000
commit3fe900e7b6808a214b3341bf923bd57a67ce9450 (patch)
tree54c3c92a17618328e021c2b9b21d27c2f9116c9a /param.ccl
parent52ed503635a6c5dc06bd8bd8866b6eb6f00ec28b (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.ccl16
1 files changed, 16 insertions, 0 deletions
diff --git a/param.ccl b/param.ccl
index e042819..b93b451 100644
--- a/param.ccl
+++ b/param.ccl
@@ -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