| Commit message (Collapse) | Author | Age |
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really all I need is that this happens only once. Allocation was already
protected by a grid scalar, unfortunately deallocation did not check/reset
this scalar
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@301 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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otherwise unallocated memory is accessed
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@300 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* fix some indices
* move poison loop to proper spot
* compute conserved divergence in track_divB
* add Maple worksheet to check constraint transport indices
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@298 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@297 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@296 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@294 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@293 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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used/allocated already anyway
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@292 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@289 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@288 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@287 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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This affects only GRMHD tests. SRMHD ones are safe.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@284 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@283 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this only shows up if we use a general eos (not a polytype) during evolution
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@282 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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for catching this up too.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@280 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@279 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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this is need for gfortran 4.1 which otherwise assumes that the arrays have
already been used (in the kind(gaa) initializations inside of
CCTK_DECLARE_ARGUMENTS).
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@278 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@277 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@276 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@275 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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GRHydro now compiles and runs without MP thorns present and behaves
identical to the old version
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@274 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* 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
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@272 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* 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
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original commit by Christian Ott (cott)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@268 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* fix con2prim issues (pertaining to error messages)
* fix OMP CRITICAL issues in Prim2Con and Con2Prim
original commits by Christian Ott (cott)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@267 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@266 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@262 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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a routine that is scheduled in BASEGRID after ADMBase sets the shift
state.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@261 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@257 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* get rid of nonsensical re-computation of the conserved tracer
* remove support for shift_state = 0 and get rid of unnecessary
assignments.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@256 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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Comments:
1) The reconstruct routine is the most expensive routine
in GRHydro and may require some serious thought in the
future regarding optimization.
2) This routine was merged by the end of the last year.
With too many loops, the compiler wasn't able to fully
optimize it (and it would warn about that).
3) With this split, the code became easier to read,
the compiler was able to fully optimize it, but we only
have a marginal gain in the routine performance (3.2%).
Further optimization and clean-up is still desirable.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@252 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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hot EOS with an atmosphere
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@249 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@248 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@245 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@226 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* 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
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@224 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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* test suites pass
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@223 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@221 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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multiple WORKSHARE sections are used since the standard does only seem to
allow assignments and WHERE statements in WORKSHARE sections
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@220 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@219 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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