The $ν$MSM, Inflation, and Dark Matter

Details The $ν$MSM, Inflation, and Dark Matter The $ν$MSM, Inflation, and Dark Matter

2006-04-27

arxiv.org/abs/hep-ph/0604236v2

Phys.Lett.B639:414-417,2006

Physics

High Energy Physics

High Energy Physics - Phenomenology

9 pages, misprints corrected, final version appeared in Phys. Lett

Scientific paper

10.1016/j.physletb.2006.06.063

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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