GRHydro.git - [no description]

	Commit message (Collapse)	Author	Age
*	GRHydro: pass pressure into eigenvalue routine for MHD	rhaas	2013-03-28
\| \| \| \| \| \| \| \|	bugfix for hot eos case, just more efficient for cold eos From: Roland Haas <rhaas@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@496 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
*	GRHydro: remove unused variables	rhaas	2013-03-28
\| \| \| \| \| \|	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: Changes to make GRHydro MHD work with nuclear/hot equation of state:	rhaas	2012-08-27
\| \| \| \| \| \| \| \| \| \| \| \| \| \| \| \| \| \|	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
*	* make EOS Omni calls thread safe	cott	2010-12-21
\| \| \| \|	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 r185	knarf	2010-11-26
\| \| \| \|	git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@186 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
*	Current RIT GRMHD code contributions:	bmundim	2010-09-29
	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