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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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to include Tmunu in the count. Extra constraints are cheap since MoL
does not allocate any scratch or save storage for them.
Bruno Mundim pointed this one out and provided the accurate count.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@373 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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evolve_MHD""
Ahem. I had reverted the wrong commit. This one was blameless.
This reverts commit 0b5a561872841b50ea32da2b665a04b2984a8c16.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@371 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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This reverts commit c2122aa2b4762388eb90cc159750aa4d418b112d.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@370 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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This reverts commit f9f8bffea9d960fb9f20cd3fe09ca9460b247adb.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@369 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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This reverts commit 6acb4ef4a535279e58f4041dc06d39c4eaf590a0.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@368 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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none"
This reverts commit 7f01f5ce8acd6d03a3dd44637f627a17eb37c120.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@367 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this fixes the aborts by Carpet for vertex centered simulations in which
it complained about the wrong order of prolongation being used.
Me culpa, since I suggested using "copy" rather than "none".
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@366 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@365 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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initializing a variable makes it SAVE which is incomaptible with OpenMP.
Also fix some 1-element-array vs. scalar variable type issues.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@364 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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with EOS tables that don't extend sufficiently far. Enforcement happens in Con2Prim.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@363 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@362 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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eigenvalue routine.
the previous patch with this same commit message (r359) has the wrong commit message.
It should instead read:
--8<--
Introduce real-valued atmo mask that can be interpolated. Synchronize
real-valued atmo mask and update integer-valued atmo mask based on synchronized
value. This fix ensures that the results are independent of the number of
processors used. It also gets rid of some extra primitive syncs that are
otherwise necessary when sync_conserved_only = yes.
Does not cause any new test failures (Roland).
Patch by Christian Reisswig.
--8<--
Patch by Christian Ott.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@361 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@360 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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It was set to +-c when it should be the maximum coming from the constraint
that the normal vector to the characteristic hypersurface of a wave
propagating along an arbitrary x direction be spacelike. This results
into the following bound for the wavespeed:
+- \alpha sqrt(\gamma^{xx}) - \beta^x)
Patch by Bruno Mundim.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@358 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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gfortran (and the Fortran standard I guess) does not allow this.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@357 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Patch by Christian Ott.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@356 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@355 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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activated if user requested this.
Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@354 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Thanks to Ian Hinder for pointing these (and the last one) out.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@353 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@352 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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there is a related patch in TRAC at the moment
Patch by Josh Faber.
Some additional checks by Roland Haas.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@351 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@350 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@349 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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on coarse reflevels via GRHydro_c2p_warn_from_level
parameter.
Patch by Christian Ott.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@348 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Note: This should be propagated to ET!
Patch by Christian Ott.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@347 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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projecting out non-radial parts of the conserved
velocity RHSs.
Patch by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@346 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this is useful when running with a spacetime code that will register
the ADMBase variables as constrained anyway, so one can save the
memory used for SandR scratch space.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@345 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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This saves some syncs. This also gets rid of the akward parameter
"disable_sync_and_tmunu_after_mol".
Original patch by Christian Reisswig.
Adapted to not rely on MoL support by Roland Haas.
Bug fixed by Christian Reisswig.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@343 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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