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* GRHydro: explicitly recompute SqrtDetg after RECOVERYrhaas2013-08-13
| | | | | | | | | this is usually not required, unless MoL_run_MoL_PostStep_in_PostRecoverVariables is set to false. From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@565 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: fix metric GF used for sqrtdetg in multipatch runsrhaas2013-08-13
| | | | | | | | fix some scheduling From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@564 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Implemented WENO-z. Ability to choose between standard WENO5 and ↵rhaas2013-08-13
| | | | | | | | "adaptive epsilon"-variant from WHAM. From: Christian Reisswig <reisswig@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@563 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: always set up SqrtDetg GF in INITIALrhaas2013-07-15
| | | | | | | | | rather than only when evolution_method == "GRHydro" so that ID only runs (or static) runs can use InitialAtmosphereReset From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@562 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: activate storage for Y_e, temperature, entropy when we evolve itrhaas2013-07-06
| | | | | | From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@558 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: add grid function for sqrt(detg)rhaas2013-07-06
| | | | | | | | | | * add new 1 tl grid function sdetg that stores the sqrt of the determinent of the 3-metric. * replace lots of re-computation of det by use of this grid function From: Christian Ott <cott@bethe.tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@555 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Make "CalcBcom" compatible with multipatch by enforcing scheduling ↵rhaas2013-07-06
| | | | | | | | after local->global trafo of primitives. From: Christian Reisswig <reisswig@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@546 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: implemented H viscosity for HLLE solver to eliminate the carbuncle ↵rhaas2013-03-28
| | | | | | | | instability. Tested with shocktube and TOV. Not yet tested for problem where carbuncles occur. From: Christian Reisswig <reisswig@scriwalker.(none)> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@491 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: synchronize press for initial guess of Con2Primrhaas2013-02-11
| | | | | | | | | | | | 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
* * add option to reconstruct temperature to GRHydrorhaas2013-02-11
| | | | | | | | | | | | 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
* GRHydro: Implemented WENO5. Tested with a shock tube.rhaas2013-01-14
| | | | | | From: Christian Reisswig <reisswig@scriwalker.(none)> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@465 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Starting to push vector potential changesrhaas2013-01-14
| | | | | | | | | | * 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
* GRHydro: Add basic vector potential supportrhaas2013-01-14
| | | | | | | | | | 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
* GRHydro: Implement entropy evolution (separated from temp evolution)rhaas2013-01-14
| | | | | | 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
* GRHydro: use timelevels parameter in STORAGE statementrhaas2013-01-14
| | | | | | | | 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
* GRHydro: clean up schedule - no-op changesrhaas2013-01-14
| | | | | | | | 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
* GRHydro: undo revision 426 since it causes test failures since poltytropes userhaas2012-10-25
| | | | | | | pressure as an initial guess git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@428 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Don't sync Lorentz factor and pressure since they are always ↵rhaas2012-10-25
| | | | | | | | 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
* use an early atmosphere reset to ensure past timelevels are initialized ↵knarf2012-10-23
| | | | | | 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
* put { on new line after elseknarf2012-09-04
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@420 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Option to use the slow sector of multirate RK methods.rhaas2012-08-04
| | | | | | | | 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
* GRHydro: schedule AtmosphereReset before PrimitiveInitialGuessesBoundariesrhaas2012-07-17
| | | | | | | | 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
* * schedule GRHydroCopyIntegerMask in POST_RECOVER_VARIABLES before ↵rhaas2012-07-17
| | | | | | | | | | | 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
* GRHydro: fix apparent typos in scheduling of GRHydro_InitAtmosMaskrhaas2012-07-05
| | | | | | | | 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
* GRHydro: copy integer atmosphere mask in Post_Recover_Variablesrhaas2012-07-05
| | | | | | | | | | | 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
* GRHydro: text-only typos in schedule descriptionrhaas2012-07-05
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@381 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Fixed mislabeled scheduling comment (cosmetic change).rhaas2012-07-05
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@379 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Sync ALL prinmitives after regridding. This ensures that all ↵rhaas2012-07-05
| | | | | | 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
* GRHydro: Fixes to atmosphere mask and the way we sync.rhaas2012-07-05
| | | | | | | | | | | | | 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
* Revert "* improve handling of cs2 < 0 in the "standard" (non-MHD, non-hot ↵rhaas2012-06-22
| | | | | | | | | | 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
* Revert "GRHydro: Fix a scheduling issue related to previous atmosphere patch."rhaas2012-06-22
| | | | | | This reverts commit f9f8bffea9d960fb9f20cd3fe09ca9460b247adb. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@369 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Fix a scheduling issue related to previous atmosphere patch.rhaas2012-06-21
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@362 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * improve handling of cs2 < 0 in the "standard" (non-MHD, non-hot EOS) ↵rhaas2012-06-20
| | | | | | | | | eigenvalue routine. Patch by Christian Ott. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@359 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Added option to constrain evolution to 1D byrhaas2012-06-05
| | | | | | | | | | 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
* GRHydro: Schedule AtmosphereReset in LAST Mol_PostSteprhaas2012-06-05
| | | | | | | | | | | | 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
* GRHydro: Added parameter to perform sync on conserved quantities only.rhaas2012-06-05
| | | | | | | | | | | | | | 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
* GRHydro: fixes for GRMHDrhaas2012-05-14
| | | | | | | | | | | | | | | | | | | | All by Philipp Moesta. 1) Fix parity of psidc and divb 2) Fix a wrong index in the source terms of scon 3) Fix wrong indices of derivatives of space-time metric in the source of the divergence cleaning scalar. 4) Calculate divergence of B in MoL PseudoEvolution and set its Prolongation="Restrict". 5) Correct the source terms and fluxes for the Bfield and the divergence cleaning field when having a non-flat space-time. 6) Make sure alpha factors match between UpdateCalculation and fluxes definition. 7) Include 1/sqrt(detg) factor in calculation of \epsilon^{\muijk} in the cross product to obtain the Bfield form the vector potential. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@330 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Add a routine to calculate mag pressure/comoving fieldbmundim2012-01-03
| | | | | | | | | | * When Tmunu is not calculated, ie when no storage is selected, the comoving magnetic field/magnetic pressure wasn't calculated at all. This commit allows that now. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@310 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Use 3 time levels for bcom et al.bmundim2011-12-06
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@308 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* allocate/deallocate ENO scalars in global moderhaas2011-11-21
| | | | | | | | | | really all I need is that this happens only once. Allocation was already protected by a grid scalar, unfortunately deallocation did not check/reset this scalar git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@301 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* second iteration of constraint transportrhaas2011-11-04
| | | | | | | | | | * fix some indices * move poison loop to proper spot * compute conserved divergence in track_divB * add Maple worksheet to check constraint transport indices git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@298 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* First try of a constraint transport scheme for unigridrhaas2011-11-02
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@296 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT dev: Fix tensor parity tags for bcom and Bcons. Add prolongation tag for ↵bmundim2011-11-02
| | | | | | bcom git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@295 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* dump the atmosphere bitmask in favor of the atmosphere integer mask which is ↵knarf2011-11-01
| | | | | | used/allocated already anyway git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@292 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* remove explicit dependence on Multipatch thornsrhaas2011-09-15
| | | | | | | | | 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
* add Multipatch support to GRHydrorhaas2011-09-15
| | | | | | | | | | | * 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
* introduce optimization that allows to turn off therhaas2011-09-15
| | | | | | | | | | additional sync/settmunu after MoL is done. This will work only in runs that do not use an atmosphere. original commit by Christian Ott git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@269 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Schedule certain items before MoL_PostStepModifyeschnett2011-08-19
| | | | | | | | Schedule all those items which were scheduled "before MoL_PostStep" also "before MoL_PostStepModify". git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@265 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* re-add update of Tmunu after AtmosphereReset, fix typo in routine namerhaas2011-08-05
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@264 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * move check of shift_state .ne. 0 tocott2011-08-03
| | | | | | | | | 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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