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The $\nu$MSM, Inflation, and Dark Matter

Authors
  • Shaposhnikov, Mikhail
  • Tkachev, Igor
Type
Published Article
Publication Date
Aug 03, 2006
Submission Date
Apr 27, 2006
Identifiers
DOI: 10.1016/j.physletb.2006.06.063
arXiv ID: hep-ph/0604236
Source
arXiv
License
Unknown
External links

Abstract

We show how to enlarge the $\nu$MSM (the minimal extension of the standard model by three right-handed neutrinos) to incorporate inflation and provide a common source for electroweak symmetry breaking and for right-handed neutrino masses. In addition to inflation, the resulting theory can explain simultaneously dark matter and the baryon asymmetry of the Universe; it is consistent with experiments on neutrino oscillations and with all astrophysical and cosmological constraints on sterile neutrino as a dark matter candidate. The mass of inflaton can be much smaller than the electroweak scale.

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