| Commit message (Collapse) | Author | Age |
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correctly. This does not work for relative settings, but at least for absolute ones. See ticket #1071 for more information
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@423 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Found by Frank Loeffler.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@422 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@421 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@420 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@419 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@418 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@417 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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the primitive velocity 'vel'.
This ensures that the Lorentz factor can never become unphysical during reconstruction.
This patch is necessary for NS collapse when ePPM+Refluxing is used.
The idea is due to Roland.
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@416 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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1) Set correct keytemp in C2P
2) Fix OpenMP private variable declaration in HLLEM
3) Fix velocity arguments for Y_e 1D PPM reconstruction
4) If in atmosphere and if evolve a Y_e also reset Y_e with cell averaged value in Reconstruction
5) Fix index permutation bug in ReconstructPoly routines for divergence cleaning field
6) Remove extra comment character in UpdateMaskM
7) Fix a missing velocity permutation when calling 1D reconstruction for Y_e.
8) Insert missing sqrt(det) factor for pressure term in resetting tau when temperature got too cold with a hot EOS.
From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@415 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@414 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* improve error handling in C2P hot routine
* further bugfix to tau reset treatment in hot part
* fix an inconsistency in hot-EOS Con2Prim routine -- when resetting
utau, also reset tau for consistency
From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@413 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@412 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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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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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@409 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@408 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@407 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@406 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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NOTE: This patch requires support from MoL.
Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@405 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Move MPI support from flesh to thorn ExternalLibraries/MPI. This also
requires thorns that call MPI directly to declare this in their
configuration.ccl. Existing configurations using MPI need to include
ExternalLibraries/MPI into their thorn list.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@404 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@403 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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I appreciate the effort to make the code compile with gcc by no longer
using integers in place of logicals. I really do. However it seems that
F0RTRAN in its infinite wisdom requires you to write
... .and. mustbisect .eqv. .true.
(note the all important 'v') when testing logicals. I have instead opted
to remove the whole .eqv. term in favor of
... .and. mustbisect
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@402 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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associated with NS collapse test case when full GR is used.
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@401 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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which used to be called PrimitiveBoundaries
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@400 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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MoL_PostStep rather than HydroBase_PostStep, since the latter is scheduled IN MoL_PostStep
-> rely on correct scheduling rather than on luck to get the correct
atmosphere map after recovery.
From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@399 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@398 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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metric.
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@397 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@396 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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patch)
From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@395 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@394 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@393 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@392 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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No actual data was updated.
data was generated without sync_only_primities but we compare against
sync_only_primitives which was always the intend of the test.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@391 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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to maek it compiel on Kraken without specifying -openmp to the linker
and complaining about ifcore vs ifcoremt issues
sort object file before library files for static linkage avoid compiler
warning about using libm math rather than mkl math
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@390 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@389 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this was harmless since the pointers to grid functions affected were OMP
shared anyway
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@388 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@387 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@386 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@385 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this only matters if wk_atmosphere is used and is based on the argument
that it makes no sense to do this in postrestrictinitial (at least when
vertex centering is used) but makes sense in postregridinitial
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@384 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this is required since the real valued atmosphere mask is not
checkpointed. It is valid since atmosphere_mask_real is non-zero
wherever atmosphere_mask is non-zero due to GRHydroUpdateAtmosphereMask
and atmosphere_mask is non-zero wherever atmosphere_mask_real is
non-zero because of GRHydroPostSyncAtmosphereMask, ie. the two masks are
non-zero/zero at the same points.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@383 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@382 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@381 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@380 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@379 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@376 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@375 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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since the Fortran standard does not allow this and gfortran 4.7 actually
chokes on it.
Pointed out by Erik Schnetter.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@374 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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