| Commit message (Collapse) | Author | Age |
|
|
|
|
|
|
|
|
|
|
| |
* 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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@272 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
| |
* 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
|
|
|
|
|
|
|
|
| |
original commit by Christian Ott (cott)
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@268 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
|
| |
* 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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@266 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@262 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@257 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
|
| |
* 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
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
| |
hot EOS with an atmosphere
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@249 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@248 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@246 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@245 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@244 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@226 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
| |
* 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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@224 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
| |
* test suites pass
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@223 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@221 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@219 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
| |
Lorentz factor variable from GRHydro to HydroBase
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@218 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
| |
function declaration of prim2con_hot
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@217 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@216 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@215 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@210 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@207 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
| |
to interface definition of EOS_Omni functions
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@204 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
| |
from a given reflevel
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@201 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@200 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@197 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
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
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@195 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@194 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@193 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|
|
|
|
| |
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinEvolve/GRHydro/trunk@192 c83d129a-5a75-4d5a-9c4d-ed3a5855bf45
|