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* GRHydro: no longer compute speed of sound twice in F90 MHD coderhaas2014-04-15
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@641 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: disable warnings in Prim2ConM and only set mask in Con2PrimMrhaas2014-04-15
| | | | | | | We don't abort in ptwise C2P call with MHD so that we can check for the mask and abort if necessary. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@638 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: use temperature in MHD prim2conrhaas2014-04-15
| | | | | | | | | | | this uses tempplus/tempminus in MHD prim2con this helps when temperature is actually reconstructed. It *does* however change the results already when temperature is not reconstructed, though it does make the results use constant values rather then averages which is lower order. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@634 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: make routine to compute speed of sound callable from F90 MHD p2crhaas2014-04-15
| | | | | | | the code is long and complicated enough that it should better not be copied and pasted. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@633 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: use ashX instead of lsh(X) when declaring array sizesrhaas2013-10-29
| | | | | | | | 1.) one should use ash when declaring array sizes 2.) intel11 chokes on lsh(X), this was already in the first Cray pointer patch git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@585 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: replace Fortan pointers with Cray pointersrhaas2013-10-27
| | | | | | | Intel 12 seems to like these better. Otherwise GRHydro_Con2PrimM.F90 takes very long to compile. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@580 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Adjust loops for Prim2Con call (needs to run in the ghost zones as well ↵HEADmasterrhaas2013-08-13
| | | | | | | | after being called from ZelmaniLeak). From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@579 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: pass correct temperature o prim2con call on coarse levelsrhaas2013-07-06
| | | | | | | | | Fix a bug in prim2con_hot that was causing temp to go negative near the shock in 3D CCSN simulations with WENO reconstruction. From: abdik <abdik@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@554 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Make MHD version of Prim2Con compatible with multipatch.rhaas2013-07-06
| | | | | | From: Christian Reisswig <reisswig@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@544 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Fix a problem with ghost zones in Prim2ConCells calls in MHD case.rhaas2013-05-11
| | | | | | From: Christian Reisswig <reisswig@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@512 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: move critical section in prim2conM into if statementrhaas2013-03-28
| | | | | | | | | otherwise the code will enter and leave the critical section during each loop iteration From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@499 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: remove unused variablesrhaas2013-03-28
| | | | | | From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@495 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: output v2 when warning about NaN in w_lorentzrhaas2013-01-14
| | | | | | 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
* 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: Introduce GRHydro_tau_min = 10^-10 max(tau(t=0)) to be used in tau ↵rhaas2012-11-09
| | | | | | | | 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
* GRHydro: add extensive information output to check_C2P_failedrhaas2012-11-09
| | | | | | From: Roland Haas <roland.haas@physics.gatech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@432 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Changes fixing issues with hot EOS treatment:rhaas2012-08-27
| | | | | | | | | | | | | | | 1) Set correct keytemp in C2P 2) Fix OpenMP private variable declaration in HLLEM 3) Fix velocity arguments for Y_e 1D PPM reconstruction 4) If in atmosphere and if evolve a Y_e also reset Y_e with cell averaged value in Reconstruction 5) Fix index permutation bug in ReconstructPoly routines for divergence cleaning field 6) Remove extra comment character in UpdateMaskM 7) Fix a missing velocity permutation when calling 1D reconstruction for Y_e. 8) Insert missing sqrt(det) factor for pressure term in resetting tau when temperature got too cold with a hot EOS. From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@415 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* GRHydro: Changes to make GRHydro MHD work with nuclear/hot equation of state:rhaas2012-08-27
| | | | | | | | | | | | | | | | | | 1) Switch to EOSOmni pointwise C2P routine and modify where necessary. 2) Modify Con2PrimM.F90 to allow for the evolution of temperature and adjust the wrapper routine. 3) Create EigenProblemM_hot pointwise routine and call that from HLLEM.F90 when temperature is evolved. Additionally adjust HLLEM where necessary. 4) Adjust InterfacesM.h to incorporate the newly created functions. 5) Fix a loop problem (not taking into account constraint transport) in PPM reconstruction of Y_e 6) Introduce Prim2ConM_hot and call this pointwise routine from Prim2ConM.F90 when temperature is evolved. Additionally also make this routine available to initial data routine in GRHydro_InitData 7) Adjust loops in GRHydro_PoloidalMagFieldM.F90 to not set boundary points it cannot set but instead call boundary group afterwards! Pay attention as this will not work with boundary conditions set to "none" in MHD case anymore but is the correct thing to do. 8) Allow StarMapper to extend HydroBase::initial_hydro = "starmapper". 9) Smaller fixes. From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@410 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* expand region where fluxes are computed for constraint transportrhaas2011-11-29
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@307 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Declare all OpenMP private variables explicitly as privateeschnett2011-06-13
| | | | | | | | | In Fortran OpenMP, loop variables of parallel loops are implicitly private and do not need to be declared as private. To improve code clarity, all such variables are now explicitly declared to be private. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@251 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
* Josh's fix for prim2conMbmundim2011-04-28
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@245 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
* * 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
* 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
* * make EOS Omni calls thread safecott2010-12-21
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@194 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
* Correct inconsistent argument list in call to prim2conpolytypeMeschnett2010-10-04
| | | | git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@159 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
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