| Commit message (Collapse) | Author | Age |
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<git@github.com:ianhinder/Kranc.git>.
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grid function
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Conflicts:
ML_BSSN/src/ML_BSSN_Minkowski.c
ML_BSSN/src/ML_BSSN_convertFromADMBase.c
ML_BSSN/src/ML_BSSN_convertFromADMBaseGamma.c
ML_BSSN/src/ML_BSSN_setBetaDriverSpatial.c
ML_BSSN/src/make.code.defn
ML_BSSN_Helper/src/SetGroupTags.c
ML_BSSN_M/param.ccl
ML_BSSN_M/schedule.ccl
ML_BSSN_M/src/ML_BSSN_M_Minkowski.c
ML_BSSN_M/src/ML_BSSN_M_convertFromADMBase.c
ML_BSSN_M/src/ML_BSSN_M_convertFromADMBaseGamma.c
ML_BSSN_M/src/ML_BSSN_M_setBetaDriverSpatial.c
ML_BSSN_M/src/make.code.defn
ML_BSSN_MP/src/ML_BSSN_MP_Minkowski.c
ML_BSSN_MP/src/ML_BSSN_MP_convertFromADMBase.c
ML_BSSN_MP/src/ML_BSSN_MP_convertFromADMBaseGamma.c
ML_BSSN_MP/src/ML_BSSN_MP_setBetaDriverSpatial.c
ML_BSSN_MP/src/make.code.defn
ML_BSSN_MP_Helper/src/SetGroupTags.c
ML_BSSN_M_Helper/schedule.ccl
ML_BSSN_M_Helper/src/SetGroupTags.c
m/McLachlan_BSSN.m
m/prototype/ML_BSSN_Helper/src/SetGroupTags.c
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CCTK_POST_RECOVER_VARIABLES
-> recompute ADM variables after recovery before first timestep
Signed-off-by: Frank Loeffler <knarf@cct.lsu.edu>
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Schedule BetaDriver setup routines in initial, postregrid and
post_recover_variables.
Signed-off-by: Peter Diener <diener@linux-hn3d.site>
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Signed-off-by: Peter Diener <diener@linux-hn3d.site>
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LSUThorns/NewRad.
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before the first time step if they have multiple time levels.
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ssh://relativity.phys.lsu.edu/home/perturbed/gitroot/McLachlan
Conflicts:
m/Makefile
m/McLachlan_BSSN.m
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Kranc does this on its own. Correct instead an error in Kranc which
registers the symmetries too late.
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This allows using octant mode and other symmetries of CartGrid3D.
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the ADMBase variables are calculated at every substep in MoL_PostStep, or
only once at CCTK_EVOL, or only once at CCTK_ANALYSIS.
Remove unused calculation convertToADMBaseLapseShiftCalc.
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ML_BSSN_MP for multi-patch simulations, and ML_BSSN_M for AMR simulations
with matter.
Add helper thorns for all BSSN thorns. Helper thorns are required at run
time, e.g. to register gauge conditions.
Split ADM and BSSN equations into their own source files.
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