| Commit message (Collapse) | Author | Age |
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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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From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@481 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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since the Polytype (!) con2prim routine uses it for its initial guess
then continues to iterate over rho
Do not sync variables not used for initial guess. This affects only runs
with sync_only_conservatives=yes.
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@480 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: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@477 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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evolution_mask is every only set to 0d0 or 1d0 (explicitly) right now.
Should this change, this tests needs to be amended.
From: Roland Haas <rhaas@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@474 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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This does not yet work with the MHD part of the code,
but Philipp is going to change this.
* Improve TOVSolverHot; in particular, give functions unique
names to avoid duplicate symbols with TOVSolverC
From: Christian Ott <cott@bethe.tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@473 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@472 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@470 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@468 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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according to WHAM code paper, (ii) Catch epsilon<0 for non-microphysical EOS. Tested with shock tube and TOV.
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@466 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@465 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@464 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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also check actual timelevels information for storage of bcom
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@463 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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before a term rho*b2 was present when the correct one is only b2
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@462 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@461 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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> \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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* 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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* faster falloff to make sure to damp to atmosphere at
Tmunu_damping_radius_max
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@457 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Basic cell-centered, algebraic gauge vector potential
method with place-holders for lorenz gauge.
Initial Avec constrained to poloidal at the moment.
From: Tanja Bode <tanja.bode@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@456 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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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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radius. Off by default.
From: Christian Reisswig <reisswig@scriwalker.(none)>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@453 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@452 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@451 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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use previous primitive values and get the cons from them. Basically freezing their values at previous time step.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@450 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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upon inversion failure of gamma law eos.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@449 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@448 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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InitialAtmosphereReset(M) so that the ID thorns do not have to know
about he excised region.
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@447 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@446 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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rather than if cascade to test for each value
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@445 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@444 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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these mostly refer to groups that used to exist but no longer do
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@443 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@442 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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unused and trigger warnings, but might be useful for debugging
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@441 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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convert type, use int which does both -> silences compiler warning
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@440 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Introduce temporary prim variables as well.
* Please refer to Illinois' paper (arXiv:1112.0568) appendices for details.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@439 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Only do this deep inside the horizon.
Reset it to conformally flat if it isn't.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@438 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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rescaling in con2prim failures.
From: Bruno Coutinho Mundim <bcmsma@astro.rit.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@437 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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while leaving the hybrid EOS behavior unchanged
From: Josh Faber <jfaberrit@jfaber3.local>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@436 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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From: Josh Faber <jfaberrit@jfaber3.local>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@435 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@434 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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since Fortran does not allow aliased arguments
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@433 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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