McLachlan.git - [no description]

	Commit message (Collapse)	Author	Age
*	Add radiative boundary conditions	Erik Schnetter	2009-09-15
\| \| \| \|	Add dependency on GenericGD to configuration.ccl
*	Add new RHS boundary condition NewRad, implemented in the thorn ↵	Erik Schnetter	2009-09-04
\| \| \| \|	LSUThorns/NewRad.
*	Add parameter MinimumLapse to enforce a positive lapse value.	Erik Schnetter	2009-08-28
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*	Register ADM variables as constrained variables, so that MoL copies them	Erik Schnetter	2009-07-03
\| \| \| \|	before the first time step if they have multiple time levels.
*	Re-generate code after correcting a code generation error in Kranc	Erik Schnetter	2009-04-28
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*	Regenerate code	Erik Schnetter	2009-04-28
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*	Merge branch 'HEAD' of ↵	Peter Diener	2009-04-27
\|\ \| \| \| \| \| \| \| \| \| \| \| \| \| \|	ssh://relativity.phys.lsu.edu/home/perturbed/gitroot/McLachlan Conflicts: ML_BSSN_MP/schedule.ccl m/McLachlan_BSSN.m
\| *	Convert to ADM variables on all grid points, including the boundary.	Erik Schnetter	2008-08-05
\| \| \| \| \| \| \| \| \| \| \| \| \| \|	Omit the derivatives on the boundary, which only affect the time derivatives of lapse and shift. Regenerate the code.
\| *	Regenerate the code	Erik Schnetter	2008-08-04
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\| *	Correct error in schedule group name	Erik Schnetter	2008-08-01
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* \|	Update auto generated code.	Peter Diener	2009-04-27
\| \| \| \| \| \| \| \|	Signed-off-by: Peter Diener <diener@linux-hn3d.site>
* \|	Merge commit 'origin/master'	Peter Diener	2008-07-01
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\| *	Add new parameter calculate_ADMBase_variables_at, which determines whether	Erik Schnetter	2008-06-16
\| \| \| \| \| \| \| \| \| \| \| \| \| \|	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.
* \|	Merge after running script	Peter Diener	2008-07-01
\|/ \| \| \| \|	Merge generated source files after running script Signed-off-by: Peter Diener <diener@diener-3.lsu.edu>
*	Re-introduce the distinction between vacuum and matter spacetimes.	Erik Schnetter	2008-05-20
\| \| \| \| \| \|	This is convenient since Kranc cannot easily detect whether the TmunuBase have storage or not, thus requiring them to have storage at all times. Differentiating between vacuum and matter spacetime avoids this.
*	Update auto-generated code	Erik Schnetter	2008-05-12
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*	Create several specialised thorns: ML_ADM and ML_BSSN as standard cases,	Erik Schnetter	2008-04-02
	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.