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28 August 2011 to 2 September 2011
Fermilab
US/Central timezone
Slides available on Indico -- there are no formal proceedings

The WIMPy Leptogenesis Miracle

31 Aug 2011, 14:00
25m
Room 105 Kersten Physics Teaching Center

Room 105 Kersten Physics Teaching Center

Speaker

Mr Brian Shuve (Harvard University)

Description

We present a new mechanism, "WIMPy Leptogenesis", which explains the near-coincidence of the present-day dark matter and baryon energy densities in a model of symmetric dark matter. In this scenario, WIMP annihilation is the source of the lepton asymmetry, which is generated by CP- and lepton-number-violating annihilations of the dark matter. The WIMP miracle is preserved, and the overall baryon and dark matter densities are determined by the dark matter annihilation cross section, as well as CP-violating phases and the strength of interactions washing out the asymmetry. We discuss one concrete model of WIMPy leptogenesis and its implications, as well as generalizations to broader classes of models.

Presentation materials