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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.
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Update the generated code after the recent changes to Kranc.
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ssh://relativity.phys.lsu.edu/home/perturbed/gitroot/McLachlan
Conflicts:
m/Makefile
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Fixed the clean command in the Makefile
Signed-off-by: Peter Diener <diener@10-4-34-85.lsu.edu>
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Correct thorn name: Use ML_FOWaveToy instead of ML_FOWavetoy (upper case T).
Regenerate thorns after correcting error in Kranc.
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