| Commit message (Collapse) | Author | Age |
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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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@250 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@247 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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necessary, but let's see if 1.e-11 also works for the moment
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@227 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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* those using carpet now activate loopcontrol
* change GRHydro::w_lorentz to HydroBase::w_lorentz
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@222 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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Lorentz factor variable from GRHydro to HydroBase
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@218 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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function declaration of prim2con_hot
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@217 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@216 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@215 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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that handles off-the-table issues with tabulated
EOS.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@214 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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fallback option when c2p does not converge -- in this case
the pointwise c2p is called again with a lower tolerance.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@213 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@212 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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maintained to work with it.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@211 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@210 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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recent
PPM changes. Old version of the code were not affected.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@209 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Fix race conditions arising in the Con2Prim routines.
Now both GNU and Intel compilers agree on the results
for the magnetic tests.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@208 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@207 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@206 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@205 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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to interface definition of EOS_Omni functions
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@204 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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schedule entries for the case with or without evolved tracers -- the
tracers won't get synced if they are not evolved, because they don't
have storage in that case.
* add entropy to the list of variables to be synced
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@203 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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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
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from a given reflevel
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@201 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@200 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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Fix to GRHydro_RegisterVarsM.cc and allows MHD to work without Y_E bing evolved.
Add C2P polytype interface.
Change schedule.ccl to represent a more detailed version of choosing what
gridfucntions get sync'd in Boundaries depending on what is being evolved.
Un-hardwire fixed values of gamma for all MHD Con2Prim routines.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@199 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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evolved ones. In this way, the conserved variables are defined on all
grid points.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@198 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@197 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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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@195 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@194 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@193 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@192 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@191 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@190 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@188 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
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