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* * fix range error in GRHydro_Y_e_maxrhaas2012-07-05
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@376 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: increase maximum and default number of constraint variablesrhaas2012-06-26
| | | | | | | | | | 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
* * introduce parameters GRHydro_Y_e_min and GRHydro_Y_e_max to fix issues ↵rhaas2012-06-21
| | | | | | 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
* * make parameter c2p_resort_to_bisection steerablerhaas2012-06-20
| | | | | | | Patch by Christian Ott. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@356 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: C2P: resort to bisection if Newton-Raphson fails. This is onlyrhaas2012-06-20
| | | | | | | | | 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
* GRHydro: Fix slope limiters and get rid of broken cases;rhaas2012-06-05
| | | | | | | | | | | 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
* GRHydro: Make enahnced params steerable.rhaas2012-06-05
| | | | | | | | Patch by Christian Reisswig. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@349 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 verbosity parameter.rhaas2012-06-05
| | | | | | | Patch by Christian Reisswig. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@342 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
* Change default value of kap_dc from 1.0 to 10.0 as well as the recommendations.bmundim2012-05-17
| | | | | | | | | | | | | This is based on the magnetic monopole tests. It indicates that kap_dc = 10.0 reaches the best balance between damping and advecting. kap_dc = 1.0 advects well but damps much slower. kap_dc = 100.0 seems to turn the problem into a stiff one and it fails to either damp or advect the divergencies away when compared to the other two cases. The recommendation then goes to use values between 1.0 and 10.0. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@337 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: decouple Bvec(flux_direction) from other two for divcleanrhaas2012-05-16
| | | | | | | | since it and psidc form a 2d subsystem of the characteristic system. See eg. Mignonoe et al. arXiv:1001.2832v2 section 3.1. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@335 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Cleanup of PPM routine. Remove unused PPM parameter. Only apply stricter ↵reisswig2012-05-14
| | | | | | "beyond Colella" limiting scheme to epsilon (to avoid that correction in one step leads to negative values). git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@333 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* epsilon: specific internal energy (ie energy/mass)bmundim2012-03-13
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@315 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Implemented enhanced PPM scheme by Colella & Sekora 2008, McCorquodale & ↵reisswig2011-11-26
| | | | | | | | | | | | Colella 2011. Can be actived by setting use_enhanced_ppm = yes. Also fixed a bug in GRHydro_Reconstruct.F90 when using MP. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@302 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
* Adding calc_bcom parameterjfaber2011-11-01
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@291 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT dev: Implement local Lax-Friedrichs flux calculation (MHD only).bmundim2011-10-03
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@281 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
* * improve behavior of CoreCollapseControl upon recoveryrhaas2011-09-15
| | | | | | | | * improve handling of too-low temperatures in GRHydro git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@270 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
* add option to smoothly dampen Tmunu to vacuum outside of a given radiusrhaas2011-09-15
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@266 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* RIT GRMHD dev:bmundim2011-08-04
| | | | | | | | | | Change legacy divergence cleaning parameters ch_dc and cp_dc, introduced for the special relativistic case, to kap_dc, the one introduced in the covariant formulation (Liebling et al.). git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@263 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
* * add new parameters for hot EOS atmosphere handlingcott2011-06-11
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@250 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
* * update to hot c2p routine: allow for a failsafe modecott2011-02-06
| | | | | | | | | that handles off-the-table issues with tabulated EOS. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@214 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
* * adjustments for things to work with updatedcott2010-08-18
| | | | | | | | | | EOS_Omni interface * test case passes git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@149 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* * add two parameters to get EOS Omni working.cott2010-07-02
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@130 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
* * make parameter enabling internal excision always steerable.cott2010-04-11
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@105 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* introduce possibilty to disable internal excision mechanism and use another ↵knarf2010-04-09
| | | | | | one (whisky_enable_internal_excision) git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@102 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* add excisionknarf2010-04-06
| | | | | | | however: be carefull with ENO and excision for the time being git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@94 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* check for velocity-overshoots from reconstruction which otherwise would ↵knarf2010-02-09
| | | | | | produce NaNs, e.g. in w_lorentz. We cannot really do something against this, so we simply limit w_lorentz to some really large value, or similar git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@68 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* remove analysis routines (moved to Hydro_Analysis), removed SetDriftCorrect ↵knarf2010-01-12
| | | | | | funtions because apparently unused - could also be implemented in extra thorn if requested git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@34 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* update from public Whisky versionknarf2009-12-08
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@5 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* This is a _temporary_ repository to be able to start to work on theknarf2009-11-18
code right now. I have put in the public version of Whisky to start from. Everybody with commit rights should get commit messages (and the other way around). It should not be a problem to add people to that list, just ask. I don't want to get into political problems because someone feels excluded, but I also don't want to give everyone access per se. Frank git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@3 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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