Cosmic lepton (flavor) asymmetry — constraints and consequences

Cosmic lepton (flavor) asymmetry — constraints and consequences

After summarizing the observational constraints on lepton (flavor) asymmetry of the Universe, I will discuss several consequences a of moderately large lepton asymmetry. It will be shown that lepton asymmetry can influence the dynamics of the cosmic QCD transition and modify the abundance of WIMPs.

University of Bielefeld

Date
30 March 2011
Expired!
Time
14h15 – 0h00
Location
Salle Claude Itzykson, Bât. 774

Speaker

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