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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
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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
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From: Philipp Moesta <pmoesta@tapir.caltech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@414 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this time with minimal replacements in SourceM.F90
From: Roland Haas <roland.haas@physics.gatech.edu>
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@411 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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It was set to +-c when it should be the maximum coming from the constraint
that the normal vector to the characteristic hypersurface of a wave
propagating along an arbitrary x direction be spacelike. This results
into the following bound for the wavespeed:
+- \alpha sqrt(\gamma^{xx}) - \beta^x)
Patch by Bruno Mundim.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@358 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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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
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@307 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@281 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Cowling calculations of spherically symmetric objects, there is no reason
not to have storage for the shift).
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@259 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@246 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@244 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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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
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true content
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@189 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@186 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@161 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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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