GRHydro_InitData.git - [no description]

	Commit message (Collapse)	Author	Age
*	GRHydro_InitData: Reschedule to make things work with multipatch. Spit out a ↵	rhaas	2013-07-06
\| \| \| \| \| \| \| \| \| \|	compile-time warning since poloidal ID B-field routine is not yet adapted to MP. From: Christian Reisswig <reisswig@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@215 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	GRHydro_InitData: Add basic vector potential support	rhaas	2013-01-11
\| \| \| \| \| \| \| \|	Initial Avec constrained to poloidal at the moment. From: Tanja Bode <tanja.bode@physics.gatech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@195 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	Rename conflicting temporary Aphi	tbode	2012-11-21
\| \| \| \|	git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@188 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	Make GRHydro_PoloidalMagFieldM.F90 call P2C correctly for temperature ↵	rhaas	2012-09-04
\| \| \| \| \| \| \| \|	evolved or not evolved. From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@154 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	Changes to make GRHydro MHD work with nuclear/hot equation of state:	rhaas	2012-09-04
\| \| \| \| \| \| \| \| \| \| \| \| \| \| \| \| \| \|	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/EinsteinInitialData/GRHydro_InitData/trunk@153 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	A couple of changes:	rhaas	2012-08-09
\| \| \| \| \| \| \| \| \| \| \|	1) Calculate divergence of B in MoL PseudoEvolution and set its Prolongation="Restrict". 2) Correct the source terms and fluxes for the Bfield and the divergence cleaning field when having a non-flat space-time. 3) Make sure alpha factors match between UpdateCalculation and fluxes definition. 4) Include 1/sqrt(detg) factor in calculation of \epsilon^{\muijk} in the cross product to obtain the Bfield form the vector potential. From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@137 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	Fix a sign error in the poloidal mag field idata	rhaas	2012-08-09
\| \| \| \| \| \|	From: Philipp Moesta <pmoesta@tapir.caltech.edu> git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@136 ac85fae7-cede-4708-beff-ae01c7fa1c26
*	Snapshot of ET GRHydro_InitData rev. 132 with a poloidal magnetic field routine	rhaas	2012-08-09
	added. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/GRHydro_InitData/trunk@134 ac85fae7-cede-4708-beff-ae01c7fa1c26