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authorrhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45>2013-03-28 01:46:26 +0000
committerrhaas <rhaas@c83d129a-5a75-4d5a-9c4d-ed3a5855bf45>2013-03-28 01:46:26 +0000
commit435d20790aa1f4c0a2b0f27c50f43649bdd58f78 (patch)
tree547331d957c5e95a9e7d144416ffb54502e9928e /param.ccl
parenta3c3a120e4686c1da48ccc9a3a9556232d104c67 (diff)
GRHydro: implemented H viscosity for HLLE solver to eliminate the carbuncle instability. Tested with shocktube and TOV. Not yet tested for problem where carbuncles occur.
From: Christian Reisswig <reisswig@scriwalker.(none)> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@491 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
Diffstat (limited to 'param.ccl')
-rw-r--r--param.ccl4
1 files changed, 4 insertions, 0 deletions
diff --git a/param.ccl b/param.ccl
index 7074529..44f6b22 100644
--- a/param.ccl
+++ b/param.ccl
@@ -310,6 +310,10 @@ keyword numerical_viscosity "How to compute the numerical viscosity"
"normal" :: "Normal numerical viscosity"
} "fast"
+boolean apply_H_viscosity "H viscosity is useful to fix the carbuncle instability seen at strong shocks"
+{
+} no
+
keyword bound "Which boundary condition to use - FIXME"
{
"flat" :: "Zero order extrapolation"