1. The Enzo Project
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  3. enzo-dev

Commits

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Author Commit Message Date Builds
Brian O'Shea
Merged in brittonsmith/enzo-dev (pull request #330) Marging stable back to week-of-code
Britton Smith
Merging.
Britton Smith
Merging.
Britton Smith
Changing cellsize for cic_deposit to the grid cellwidth.
Branches
stable
Britton Smith
Merging stable back to week-of-code.
Britton Smith
Updating Blue Waters make file.
Branches
stable
Nathan Goldbaum
Add missing ErrorExceptions.h includes to fix compilation under icpc Thanks to Greg Bryan for suggesting this fix.
Brian O'Shea
Added tag enzo-2.5 for changeset 2984068d220f
Branches
stable
Brian O'Shea
merged enzo-dev with stable
Tags
enzo-2.5
Branches
stable
Brian O'Shea
updating changelog and readme with one further commit
Brian O'Shea
Merged enzo/enzo-dev into week-of-code
Brian O'Shea
updating changelog as per nathan's suggestion
Brian O'Shea
updated readme - one more email address
Brian O'Shea
updated CHANGELOG and README
Brian O'Shea
updating version numbers everywhere
Andrew Emerick
Made sure CRDiffusion only occurs with CRModel ON. Fail statement to check this at runtime.
John Wise
Merging with mainline
John Wise
Putting the number of flagged cells from MRPs in debug1 mode to be consistent with the reporting in grid::SetFlaggingField().
John Wise
Putting this code in the TRANSFER ifdef so that photon-no compiles.
shuokong
fix a bug that potentially causes segfault in 2D simulation
Brian O'Shea
Merged in gbryan/enzo-dev-mom (pull request #277) Kinetic Feedback
Cameron Hummels
Adding note in docs about failures experienced in testing with StarFeedbackKineticFraction = -1.
Cameron Hummels
Adding debug flag conditionals to avoid extraneous debug information flooding STDOUT.
Christine Simpson
Put print statements in debug option; raised lower limit on kinf
Christine Simpson
Placing floor to kinf in star_maker3mom when adaptive kinf is used to avoid precision issues
Christine Simpson
fixed index error
Christine Simpson
updates to starmaker3mom
Christine Simpson
adjusted particle dynamical time for momentum feedback in start particle test problem
Christine Simpson
put in some diagnostic print statements
Christine Simpson
corrected computation of total energy of feedback zone in the case where the dual energy formalism is not used, but neither is Zeus. In this case, after the feedback has been done (but before the end of the routine), the te field has been updated with the thermal feedback energy, but not the kinetic feedback energy. The thermal energy of the feedback region after the feedback should therefore be sum(te_i*d_i) - ke_before.
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