Scott Dodelson
Published 2008-12-03, updated 2008-12-08Version 2
A simple formula is introduced which indicates the amount by which projections of dark matter direct detection experiments are expected to be degraded due to backgrounds.
Comments: 4 pages, 3 figures, code available at http://home.fnal.gov/~dodelson/dm.html
Journal: Phys.Rev.D79:043508,2009
A universal density slope - velocity anisotropy relation for relaxed structures
A simple formula for the thermal pair annihilation line emissivity
Red Mergers and the Assembly of Massive Elliptical Galaxies: the Fundamental Plane and its Projections
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