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authorrhaas <rhaas@ac85fae7-cede-4708-beff-ae01c7fa1c26>2012-09-04 12:28:40 +0000
committerrhaas <rhaas@ac85fae7-cede-4708-beff-ae01c7fa1c26>2012-09-04 12:28:40 +0000
commit91270e519a2413c00e39aee4688765bd0e4d9ab1 (patch)
tree9af5d4df8ca80a6d53c2a810ef360de8696f55c3 /schedule.ccl
parent0f066b0ae931fffa90bc79303072891357b4f333 (diff)
Changes to make GRHydro MHD work with nuclear/hot equation of state:
1) Switch to EOSOmni pointwise C2P routine and modify where necessary. 2) Modify Con2PrimM.F90 to allow for the evolution of temperature and adjust the wrapper routine. 3) Create EigenProblemM_hot pointwise routine and call that from HLLEM.F90 when temperature is evolved. Additionally adjust HLLEM where necessary. 4) Adjust InterfacesM.h to incorporate the newly created functions. 5) Fix a loop problem (not taking into account constraint transport) in PPM reconstruction of Y_e 6) Introduce Prim2ConM_hot and call this pointwise routine from Prim2ConM.F90 when temperature is evolved. Additionally also make this routine available to initial data routine in GRHydro_InitData 7) Adjust loops in GRHydro_PoloidalMagFieldM.F90 to not set boundary points it cannot set but instead call boundary group afterwards! Pay attention as this will not work with boundary conditions set to "none" in MHD case anymore but is the correct thing to do. 8) Allow StarMapper to extend HydroBase::initial_hydro = "starmapper". 9) Smaller fixes. From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@153 ac85fae7-cede-4708-beff-ae01c7fa1c26
Diffstat (limited to 'schedule.ccl')
-rw-r--r--schedule.ccl6
1 files changed, 5 insertions, 1 deletions
diff --git a/schedule.ccl b/schedule.ccl
index 2b72ab4..4bca6fc 100644
--- a/schedule.ccl
+++ b/schedule.ccl
@@ -245,9 +245,13 @@ if (CCTK_EQUALS(initial_hydro, "magnetized_bondi_solution"))
if (CCTK_EQUALS(initial_Bvec, "poloidalmagfield"))
{
- SCHEDULE GRHydro_PoloidalMagFieldM IN HydroBase_Initial AFTER TOV_Initial_Data
+# SCHEDULE GRHydro_PoloidalMagFieldM AT CCTK_INITIAL AFTER IN HydroBase_Initial AFTER rnsid_init AFTER TOV_Initial_Data after CCCC_StarMapper_InitialData
+ SCHEDULE GRHydro_PoloidalMagFieldM AT CCTK_POSTINITIAL
{
LANGUAGE: Fortran
} "Set up a poloidal magnetic field. It expects the other fluid variables already to be set, as for example in the TOV solution"
+ SCHEDULE group HydroBase_Boundaries IN HydroBase_Initial AFTER GRHydro_PoloidalMagFieldM
+ {
+ } "Call boundary conditions after magnetic field initial data setup"
}