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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@656 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@655 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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the previous version would not initialize the past timelevels properly.
Unfortunately PUGH does not offer a option init_fill_levels as Carpet does, so
we use a combination of MoL and TOVSolver options to achieve the same affect.
This requires an updates MoL since the multi-rate support in MoL in rev 220 is broken.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@651 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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the tolerance is increase to the level of the 1d test
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@650 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@645 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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They were all using divergence cleaning before, however none of the
production runs ever user divergence cleaning and it is not the
recomendet choice of method.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@644 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@643 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@642 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@608 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@590 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this is a very highly relativistic shock (v=0.999) and apparently different
compilers produce very different results.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@589 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@588 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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TOV_Gamma
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@561 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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regenerate test that was using wrong stencil before
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@535 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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along the y direction. The diagonal shock causes issues near the boundary where the shock fails due to differences between gfortran and intel compilers.
One issue is obviously that the boundary condition is incorrect and one really would want to use a boundary condition similar to the ones implemented for the MHD shocks by Josh and Bruno.
For now I simplified the test which also makes to work more reliably on the different compilers.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@524 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this is just a copy of the shock tube test using MP5
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@490 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this is just a copy of the shock tube test using WENO
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@489 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@488 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@483 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@482 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* after rev 72 of EOS_Omni changed constants of nature
* increase con2prim accuracy to avoid O(1) errors in primitives due to
O(eps) changes in conservatives
* remove changes in K and Gamma to avoid setting points to atmosphere
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@479 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this affect the test_tov_carpet_refined_nosync and tov_slowsector tests.
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@478 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@476 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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remove unused Thorn from ActiveThorns.
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@475 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@471 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@469 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this fixes a test failure introduced in r454
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@467 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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tests in regions that are not needed for evolution
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@454 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@429 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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these are all based on the shocktube and cylindrical explosion tests of the ET
MHD paper of the same name.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@424 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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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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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@317 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@316 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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support removal for shift_state = 0.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@258 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@254 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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McLachlan (ML_BSSN_O2) requires two ghost/boundary points due to the dissipation and upwinded advection operators. Kranc-generated thorns now check that the correct number of ghost and boundary points are available, and this check causes three GRHydro tests to fail as they use a boundary size of 1. It turns out that if you disable the check, the original GRHydro test suite still passes on Intel with Linux (Damiana) but segfaulted on GCC with Mac OS (my laptop). The dissipation and unwinding operators will be reading off the edge of the grid, so the behavior is undefined. Dissipation is set to 0 in this test, but a nonzero shift is used. This commit sets the CoordBase boundary size to 2 in the tests, and this requires the test data to be regenerated (the following commit).
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@253 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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necessary, but let's see if 1.e-11 also works for the moment
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@227 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* those using carpet now activate loopcontrol
* change GRHydro::w_lorentz to HydroBase::w_lorentz
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@222 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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initial_atmosphere_factor
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@163 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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to worry about it. This changes the data slitely for EOSG testsuites because this now uses EOSG calls instead of the otherwise fixed calculations of the TOVSolver, thus the change of two testsuites
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@156 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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EOS_Omni interface
* test case passes
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@149 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@135 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Omni support is not compiled in.)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@133 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@127 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@126 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@125 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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