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author | rhaas <rhaas@1bdb13ef-5d69-4035-bb54-08abeb3aa7f1> | 2010-05-28 12:07:30 +0000 |
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committer | rhaas <rhaas@1bdb13ef-5d69-4035-bb54-08abeb3aa7f1> | 2010-05-28 12:07:30 +0000 |
commit | b67701b543b74be826d888cdc8b9037b770bbb61 (patch) | |
tree | 591be9928200b7665c376e172518f3866b3c098c /param.ccl | |
parent | 744ea3ab7b31622952fd9114cf481410ecfc9716 (diff) |
TOVSolver: fix computation of Lorentz factor
Use the Valencia three velocity to compute the Lorentz factor. Add references
to the definitions to code and param.ccl. Makes no difference for initial data
that is at rest, so the testsuites are unchanged.
git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinInitialData/TOVSolver/trunk@111 1bdb13ef-5d69-4035-bb54-08abeb3aa7f1
Diffstat (limited to 'param.ccl')
-rw-r--r-- | param.ccl | 3 |
1 files changed, 3 insertions, 0 deletions
@@ -63,6 +63,9 @@ CCTK_REAL TOV_Position_z[10] "Position of neutron star, z coordinate" STEERABLE= *:* :: "real" } 0.0 +# contravariant fluid three velocity as measured by the Eulerian observers: v^i = u^i / (alpha u^t) + beta^i / alpha +# as used by HydroBase. Follows the Valencia formulation eg. eqs. 26 and 27 of Font et al's paper (gr-qc/9811015) or +# below Equ. 31 in http://relativity.livingreviews.org/Articles/lrr-2008-7/articlesu1.html#x6-30002.1 CCTK_REAL TOV_Velocity_x[10] "(fixed) Velocity of neutron star, x coordinate (caution!)" STEERABLE=always { *:* :: "real" |