aboutsummaryrefslogtreecommitdiff
path: root/schedule.ccl
Commit message (Collapse)AuthorAge
* 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
* Correct scheduleeschnett2011-08-03
| | | | | | | | | | | Do not schedule group SetTmunu from GRHydro; group SetTmunu is now scheduled by thorn TmunuBase. Correct scheduling of GRHydro_AtmosphereReset, and GRHydro_AtmosphereResetM, and the associated HydroBase_Boundaries. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@260 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT GRMHD dev:bmundim2011-08-02
| | | | | | | | | | | | | | | | | | | | | | | | | | | 1) Further splitting of PPM Reconstruction routine into magnetic and non-magnetic part. 2) Merge the divergence cleaning loop into the non-divergence one, since profiling indicated no substantial difference between the two cases. Indeed it was a little bit better after the merger (0.14%), but that it is not significant. We decided then to apply Occam's razor and choose the simplest form. Branch prediction seems to work fine in this case. 3) Move reconstruction initialization statements to their repective drivers. 4) Get rid of WORKSHARE in the reconstruction routines. Profiling showed a 4.16% performance improvement for the hydro ppm reconstruction routine when using 1 processor and 2 threads only. Expect a better improvement for a larger number of threads. 5) Introduce a parameter to control characteristic speeds for psidc in HLLE. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@255 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* MERGE divergence cleaning feature into trunk.tbode2011-04-28
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@244 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT MHD development:bmundim2011-04-13
| | | | | | | | | | | | | | | 1) Fix a bug in the divergence cleaning implementation: a psidc term in the induction equation was implemented as a source term where it was supposed to be coded as part of the flux calculation. 2) Introduce divB as a diagnostic grid function. 3) Remove an old file: GRHydro_CalcUpdateM.F90 git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@228 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * remove support for "General" EOS interface (EOSG_*)cott2011-03-28
| | | | | | | | | | * test suites pass with Intel 11 (no optimizaton) on bethe and gcc 4.4.5 git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@225 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * remove GZ patch system codecott2011-03-12
| | | | | | | | * test suites pass git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@223 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * changes to go along with the move of thecott2011-02-21
| | | | | | | | | Lorentz factor variable from GRHydro to HydroBase git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@218 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * change scheduling of GRHydro_EOSHandle from local to global.cott2011-01-02
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@206 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * some more cleaning up in schedule.ccl -- we don't need separatecott2010-12-31
| | | | | | | | | | | schedule entries for the case with or without evolved tracers -- the tracers won't get synced if they are not evolved, because they don't have storage in that case. * add entropy to the list of variables to be synced git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@203 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT MHD development:bmundim2010-12-31
| | | | | | | | | | | | | | | | | | Revert previous commit changes to schedule.ccl Merge MHD and GRHydro routines: Boundaries, CalcUpdate, PPM, Reconstruct(poly), RegisterGZ, RegisterVars Solve a few race conditions arising in the "magnetic" routines. This is still being tested, since it passes tests with intel compilers but fails for gnu ones. Alias function GRHydro_Con2PrimM_pt for C2P2CM test. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@202 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT MHD dev:bmundim2010-12-25
| | | | | | | | | | | | | | | | Fix to GRHydro_RegisterVarsM.cc and allows MHD to work without Y_E bing evolved. Add C2P polytype interface. Change schedule.ccl to represent a more detailed version of choosing what gridfucntions get sync'd in Boundaries depending on what is being evolved. Un-hardwire fixed values of gamma for all MHD Con2Prim routines. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@199 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT MHD development: an update.bmundim2010-12-22
| | | | | | | | | | | | | | Several bugfixes, including properly isolating divergence cleaning code and initialization of the "psidc" gridfunction in GRHydro_DivergenceClean.F90, as well as properly initializing rhoenth in GRHydro_HLLEM (thanks to Roland for catching that). Minor changes to scheduler to properly call MHD and non-MHD routines in parallel for Riemann solving. Remove GRHydro_ParamCheckM.F90 and add GRHydro_DivergenceClean.F90. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@196 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* merge branch hot_and_MHD_temp_dev into branch at revision r185knarf2010-11-26
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@186 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT's divergence cleaning development.bmundim2010-10-12
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@161 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Current RIT GRMHD code contributions:bmundim2010-09-29
| | | | | | | | | | Add the magnetized counterparts for several GRHydro routines. Adjust interface.ccl, param.ccl and schedule.ccl appropriately. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@158 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* let GRHydro set the atmosphere of initial data, so that ID thorns don't have ↵knarf2010-09-15
| | | | | | 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
* schedule Prim2Con in HydroBase_Prim2ConInitialknarf2010-07-30
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@142 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * initial structural modifications to start with MHD development (Noble/Ott)cott2010-05-26
| | | | | | | | | | | | | | | | | | | -> add comoving b-field: bcom[3] and bcom0 -> add integer variable MHD which is set in ParamCheck to 0 or 1 according to HydroBase::Bvec_evolution_method being GRHydro or something else (don't want to do string comparisons very often) -> skeleton routine Conservative2PrimitiveM in separate .F90 file -> extend keyword Bvec_evolution_method with "GRHydro" * code compiles, should not hurt anything already there, does not do anyting (yet) git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@115 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* file/parameter string replacement from whisky to GRHydrobmundim2010-05-02
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@112 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
generated by cgit v1.2.3 (git 2.39.1) at 2024-07-01 15:54:50 +0000