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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@495 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@484 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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since only the later (a macro) contains the required ".ne. 0" to turn
the return value into a logical type
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@460 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* incl boundary calls for Avec
* disable call to BvecfromAvec from within loop, this one is a schedule
function call now.
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@458 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@455 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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pressure as an initial guess
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@428 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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computed in Con2Prim and are not needed for initial guesses.
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@426 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this time with minimal replacements in SourceM.F90
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@411 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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variables are known on the finer grid when sync_conserved_only = yes. This is fix only affects runs which use a microphysical EOS.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@378 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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These are the changes as discussed with Roland. In
particular, we sync the atmo mask in an extra call
before all other syncs and then do atmo reset.
Furthermore, primitives must always be synced in last
post step in order to get initial guesses in the
buffer zones via prolongation. Atmo reset must be
done before prolongation to ensure we don't overwrite
"good" data from the coarse grid!
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@377 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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EOS) eigenvalue routine."
actually this introduce the real valued atmosphere mask.
This reverts commit deccf528b463820b615dfa73e46e137cd59c65be.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@372 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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eigenvalue routine.
Patch by Christian Ott.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@359 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@344 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@341 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Primitives are only sync'ed after regridding to get initial guesses.
Schedule Primitive boundary call in PostRegridInitial if sync_only_coserved == yes.
Fixed issue with the sync call in CCTK_EVOL after MoL_Evolution when sync_conserved_only==yes:
Conserved vars must be synced here as well, otherwise conserved vars are reset to atmospshere whereas
primitives are not! This is wrong.
Patches by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@340 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Some variables were stil set to "Flat" boundaries even though "None" is
supposed to be set.
Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@325 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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remove unused file GRHydro_BoundariesM.F90
remove unused file GRHydro_ReconstructPolyM.F90
remove unused file GRHydro_ReconstructM.F90
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@306 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@305 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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GRHydro now compiles and runs without MP thorns present and behaves
identical to the old version
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@274 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* not all features of GRHydro are supported yet, in particular only the
HLLE solver supports Mulitpatch yet.
Original commit by Christian Reisswig and Christian Ott
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@273 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@262 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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a routine that is scheduled in BASEGRID after ADMBase sets the shift
state.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@261 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@244 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* test suites pass
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@223 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Lorentz factor variable from GRHydro to HydroBase
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@218 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Revert previous commit changes to schedule.ccl
Merge MHD and GRHydro routines:
Boundaries, CalcUpdate, PPM, Reconstruct(poly), RegisterGZ,
RegisterVars
Solve a few race conditions arising in the "magnetic" routines.
This is still being tested, since it passes tests with intel
compilers but fails for gnu ones.
Alias function GRHydro_Con2PrimM_pt for C2P2CM test.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@202 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@186 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* change calculation of the determinant of the 3-metric from
a subroutine call to a macro.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@152 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@112 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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