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McLachlan
McLachlan, a Public BSSN Code
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McLachlan is a publicly available, state-of-the-art BSSN code for solving the Einstein equations. McLachlan was created in the XiRel project, with the intention of building a public code for the numerical relativity community. McLachlan should be "good enough" for "standard" calculations of black holes, neutron stars, binary systems of these, and many other cases. McLachlan uses Kranc for code generation and is based on the Cactus framework, the Carpet adaptive mesh refinement driver, and the Einstein Toolkit. It can be combined with Whisky, the EU Network GR Hydrodynamics code.
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22:16 on Mar 18, 2010
event counters
The last message was received 4.12 days ago at 19:19 on Mar 14, 2010
0 messages so far today, 0 messages yesterday
0 messages so far this week, 4 messages last week
4 messages so far this month, 21 messages last month
25 messages since the first one, 1.27 months ago, for an average of 1.52 days between messages
recent messages
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19:18 SundayMcLachlan
Commit by schnetter :: r33479637cddf / (35 files in 13 dirs):
Correct boundary conditions
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18:14 SundayMcLachlan
Commit by schnetter :: r5e7d21dadf4c / (9 files in 7 dirs):
Schedule boundary conditions in ML_PseudoEvolution
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20:44 FridayMcLachlan
Commit by schnetter :: r213ad0628fce / (39 files in 5 dirs):
Generate and add 8th order version as well
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15:36 on Mar 09McLachlan
Commit by schnetter :: r586c78c4668b / (32 files in 11 dirs):
Make eta (the Gamma driver damping parameter) a local variable only, not a grid function
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23:30 on Feb 19McLachlan
Commit by schnetter :: r85da7a8dd591 / (67 files in 9 dirs):
Add second order accurate versions of all thorns
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21:27 on Feb 19McLachlan
Commit by schnetter :: rfa724eab3321 / (8 files in 7 dirs):
Use new schedule group MoL_PseudoEvolution for the ADM constraints and the ADM quantities.
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00:11 on Feb 14McLachlan
Commit by schnetter :: r36b4367cba09 / (35 files in 12 dirs):
Merge /Users/eschnett/Cbeta/arrangements/McLachlan
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00:11 on Feb 14McLachlan
Commit by schnetter :: r592247986d09 / (7 files in 5 dirs):
Treate Tmunu variables as tensors, instead of accessing them via local helper scalars.
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00:11 on Feb 14McLachlan
Commit by schnetter :: r76d87a0dd9b1 /m/ (Makefile McLachlan_ADMQuantities.m):
Add thorn that evaluates the kernels for global ADM quantites (ADM mass and ADM angulare momentum)
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00:11 on Feb 14McLachlan
Commit by schnetter :: r716a647adf53 /m/prototype/ML_BSSN_Helper/src/ (3 files):
Distinguish between persistent variables and those that need to be checkpointed; e.g. eta (the shift driver parameter) is persistent, but is not checkpointed.
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00:11 on Feb 14McLachlan
Commit by schnetter :: r24da23aea1e9 /m/ (2 files in 2 dirs):
Correct synchronisation problems
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00:11 on Feb 14McLachlan
Commit by schnetter :: rd895c73560eb /doc/qc0-mclachlan-public.par:
Add McLachlan's dtlapse and dtshift to output variables
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00:11 on Feb 14McLachlan
Commit by schnetter :: r7351ade3630c /m/McLachlan_ADMConstraints.m:
Add thorn that evaluates the ADM constraints
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00:11 on Feb 14McLachlan
Commit by schnetter :: r7ce13472f86f /m/McLachlan_BSSN.m:
Split RHS evaluation into two routines to reduce instruction cache usage.
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00:11 on Feb 14McLachlan
Commit by schnetter :: r1c714f0f778f /m/ (5 files):
Use relative instead of absolute path names pointing to Kranc
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00:11 on Feb 14McLachlan
Commit by schnetter :: r74c4da71a373 /m/prototype/ML_BSSN_Helper/schedule.ccl:
Remove commented out code
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00:11 on Feb 14McLachlan
Commit by schnetter :: rd589bd4b2811 /m/McLachlan_BSSN.m:
Do not generate a separate "matter" thorn; instead, the standard thorn does now handle matter terms
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00:11 on Feb 14McLachlan
Commit by schnetter :: r87973f1adaf1 /doc/checkout.sh:
Create CVS password file for anonymous checkout
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00:11 on Feb 14McLachlan
Commit by schnetter :: r0636964c3ec7 / (95 files in 15 dirs):
Merge branch 'master' of /Users/eschnett/Cbeta/arrangements/McLachlan
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00:11 on Feb 14McLachlan
Commit by schnetter :: r08571b14f158 / (7 files in 7 dirs):
Avoid division-by-zero problems when ShiftGammaCoeff=0
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