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path: root/ML_ADM/src/ML_ADM_constraints_boundary.c
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* Update auto-generated code as generated by the current version of KrancErik Schnetter2011-04-03
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* Re-generate codeErik Schnetter2011-01-03
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* Regenerate codeErik Schnetter2010-12-08
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* Regenerate codeErik Schnetter2010-10-11
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* Use Ian's version of Kranc, which is found atErik Schnetter2010-03-18
| | | | <git@github.com:ianhinder/Kranc.git>.
* Update auto-generated codeErik Schnetter2010-02-13
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* Add radiative boundary conditionsErik Schnetter2009-09-15
| | | | Add dependency on GenericGD to configuration.ccl
* Add new RHS boundary condition NewRad, implemented in the thorn ↵Erik Schnetter2009-09-04
| | | | LSUThorns/NewRad.
* Register ADM variables as constrained variables, so that MoL copies themErik Schnetter2009-07-03
| | | | before the first time step if they have multiple time levels.
* Resolve merge commitsErik Schnetter2009-04-27
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* Update auto generated files.Peter Diener2009-04-27
| | | | Signed-off-by: Peter Diener <diener@linux-hn3d.site>
* Merge commit 'origin/master'Peter Diener2008-05-15
|\ | | | | | | | | Conflicts: m/Makefile
| * Create several specialised thorns: ML_ADM and ML_BSSN as standard cases,Erik Schnetter2008-04-02
| | | | | | | | | | | | | | | | | | 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.
* | Merge commit 'origin/master'Peter Diener2008-02-13
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| * Re-generate all codeErik Schnetter2008-02-13
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* | No real changePeter Diener2008-02-13
|/ | | | | Just "produced by" comments Signed-off-by: Peter Diener <diener@diener-3.lsu.edu>
* Don't calculate ADMBase variables on the boundariesErik Schnetter2008-01-31
| | | | | Don't calculate ADMBase variables on the boundaries, since they require derivatives. Instead, select and apply boundary conditions after converting from BSSN to ADM.
* Schedule ML_BSSN_convertToADMBase everywhere.Peter Diener2008-01-29
| | | | | | | | 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>
* Update McLachlan. ML_BSSN_Helper is now required at run timeErik Schnetter2008-01-14
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.
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