Sterile neutrino dark matter as a consequence of nuMSM-induced lepton asymmetry
arXiv:0804.4543 · doi:10.1088/1475-7516/2008/06/031
Abstract
It has been pointed out in ref.[1] that in the nuMSM (Standard Model extended by three right-handed neutrinos with masses smaller than the electroweak scale), there is a corner in the parameter space where CP-violating resonant oscillations among the two heaviest right-handed neutrinos continue to operate below the freeze-out temperature of sphaleron transitions, leading to a lepton asymmetry which is considerably larger than the baryon asymmetry. Consequently, the lightest right-handed (``sterile'') neutrinos, which may serve as dark matter, are generated through an efficient resonant mechanism proposed by Shi and Fuller [2]. We re-compute the dark matter relic density and non-equilibrium momentum distribution function in this situation with quantum field theoretic methods and, confronting the results with existing astrophysical data, derive bounds on the properties of the lightest right-handed neutrinos. Our spectra can be used as an input for structure formation simulations in warm dark matter cosmologies, for a Lyman-alpha analysis of the dark matter distribution on small scales, and for studying the properties of haloes of dwarf spheroidal galaxies.
25 pages. v2: many clarifications and references added; published version
References in corpus (4)
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Cited by in corpus (7)
- Leptogenesis
- A lower bound on the mass of Dark Matter particles
- Realistic sterile neutrino dark matter with keV mass does not contradict cosmological bounds
- Right-handed neutrino magnetic moments
- Inflaton mass in the nuMSM inflation
- Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe
- Sterile neutrinos in cosmology and how to find them in the lab