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From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@578 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* add new 1 tl grid function sdetg that stores the sqrt of the determinent
of the 3-metric.
* replace lots of re-computation of det by use of this grid function
From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@555 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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This re-introduces routines that work for hybrid/hot EOS and
corresponding changes in pointwise routines for hot EOS error checking
and temperature treatment by adding old EOSOmni pointwise routine.
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@511 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@485 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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> \gamma).
not code change
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@459 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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GRHydro_Con2PrimM_pt_EOSOmni.c
* Interestingly Cactus doesn't complain about the function interface in
interface.ccl. It has the old set of arguments for that function and declare it
as written in Fortran instead of C.
* Cylindrical explosion works again with GRHydro_Con2PrimM_pt.c routine. You
can just swap both routines in make.code.defn
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@427 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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/EinsteinEvolve/GRHydro/trunk@410 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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patch by Philipp Moesta
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@324 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@289 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@288 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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