| Commit message (Collapse) | Author | Age |
|
|
| |
Reordering of entries in param.ccl due to internal cleanup in Kranc.
|
| |
|
| |
|
| |
|
| |
|
|
|
| |
Kranc version beb854b56cd60ec97072d709a064eeafe1633ed1
|
| |
|
| |
|
| |
|
|
|
|
| |
LSUThorns/NewRad.
|
| |
|
|
|
|
| |
before the first time step if they have multiple time levels.
|
| |
|
|\
| |
| |
| |
| | |
Conflicts:
m/Makefile
|
| |
| |
| |
| |
| |
| |
| |
| |
| | |
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.
|
|/
|
|
|
|
| |
dummy merge
Signed-off-by: Peter Diener <diener@diener-3.lsu.edu>
|
| |
|
|
|
|
|
|
|
|
| |
Since ML_BSSN_convertToADMBase doesn't contain any derivatives we can
evaluate it everywhere. Get's rid of a sync of the ADMBase variables and
makes it unnecessary to apply the boundary conditions (which wasn't done,
anyway).
Signed-off-by: Peter Diener <diener@diener-3.lsu.edu>
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| |
Calculate the complete RHS in one loop, including matter if desired.
This requires different McLachlan builds for runs with and without
matter.
Make the number of active timelevels a run-time parameter.
Register the slicing in ML_BSSN_Helper. This requires CoordGauge to be
activated at run time.
Add custom boundary conditions, to be used instead of Cactus boundary
conditions.
Make McLachlan fully compliant with the ADMBase initial data mechanism.
Calculate RHS and constrains in special groups provided by ML_BSSN_Helper.
ML_BSSN_Helper is now required at run time.
|
|
|
| |
Update the generated code after the recent changes to Kranc.
|
| |
|
|
|
|
|
|
| |
Fixed the clean command in the Makefile
Signed-off-by: Peter Diener <diener@10-4-34-85.lsu.edu>
|
| |
|
|
|