Viewing all changes in revision 567.
- Committer: Andrew Benson
- Date: 2012-05-29 05:12:54 UTC
- Revision ID: abenson@its.caltech.edu-20120529051254-qt2zqs4963psygfq
* Fix bug in spherical collapse calculation of virial density contrast
in dark energy cosmologies. (Ratio of final to turnaround radii was
fixed at 2 instead of being computed correctly for dark energy
cosmologies.)
in dark energy cosmologies. (Ratio of final to turnaround radii was
fixed at 2 instead of being computed correctly for dark energy
cosmologies.)
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