McLachlan.git - [no description]

	Commit message (Collapse)	Author	Age
*	Add Helper thorns that went missing during a merge (my apologies)	Erik Schnetter	2009-04-27
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*	Merge branch 'master' of ↵	Erik Schnetter	2009-04-27
\| \| \| \| \| \| \| \|	ssh://relativity.phys.lsu.edu/home/perturbed/gitroot/McLachlan Conflicts: m/Makefile m/McLachlan_BSSN.m
*	Set CartGrid3D symmetries of McLachlan's variables	Erik Schnetter	2008-08-01
\| \| \| \|	This allows using octant mode and other symmetries of CartGrid3D.
*	Update McLachlan. ML_BSSN_Helper is now required at run time	Erik Schnetter	2008-01-14
	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.