Commit message (Collapse) | Author | Age | |
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* | Remove TriggerGroups declaration | Erik Schnetter | 2012-08-17 |
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* | Don't replace Pi by its numeric equivalent -- Kranc does this already | Erik Schnetter | 2012-01-02 |
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* | McLachlan_ADM.m: Fix index errors in constraint computation | Ian Hinder | 2011-11-20 |
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* | Use kranc script instead of calling Mathematica directly | Ian Hinder | 2011-09-24 |
| | | | This allows use of better error handling provided by Kranc | ||
* | Use new fdOrder mechanism in ADM thorn | Erik Schnetter | 2011-09-23 |
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* | McLachlan_ADM.m: Add explicit "*" to quiet warning | Ian Hinder | 2011-06-29 |
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* | Use new Jacobian mechanism for all thorns | Erik Schnetter | 2011-06-23 |
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* | Rename tensor indices | Ian Hinder | 2011-06-13 |
| | | | | | | Tensor indices with numbers are not supported any more in Kranc; rename them to use letters instead. (originally by Erik Schnetter) | ||
* | Revert "Rename tensor indices" | Ian Hinder | 2011-06-13 |
| | | | | This reverts commit a8b69dc06e565427bc96d16c443bb4b3392c4365. | ||
* | Rename tensor indices | Erik Schnetter | 2011-06-12 |
| | | | | | Tensor indices with numbers are not supported any more in Kranc; rename them to use letters instead. | ||
* | Update path to Kranc | Erik Schnetter | 2010-08-04 |
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* | Use relative instead of absolute path names pointing to Kranc | Erik Schnetter | 2010-02-13 |
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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 | ||
| * | Update auto generated files. | Peter Diener | 2009-04-27 |
| | | | | | | | | Signed-off-by: Peter Diener <diener@linux-hn3d.site> | ||
* | | Add semicolons to prevent output | Erik Schnetter | 2009-04-27 |
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* | Update path to Kranc installation | Erik Schnetter | 2008-05-05 |
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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. |