ar X iv : a st ro - p h / 05 11 50 0 v 1 17 N ov 2 00 5 Is cosmology compatible with sterile neutrinos ?
نویسندگان
چکیده
By combining data from cosmic microwave background (CMB) experiments (including the recent BOOMERANG-2K2 results), large scale structure (LSS) and Lyman-α forest observations, we constrain the hypothesis of a fourth, sterile, massive neutrino. For the 3 massless + 1 massive neutrino case we bound the mass of the sterile neutrino to ms < 0.55eV at 95% c.l.. These results exclude at high significance the sterile neutrino hypothesis as an explanation of the LSND anomaly. We then generalize the analysis to account for active neutrino masses (which tightens the limit to ms < 0.51eV) and the possibility that the sterile abundance is not thermal. In the latter case, the contraints in the (mass, density) plane are non-trivial. For a mass of > 1eV or < 0.05eV the cosmological energy density in sterile neutrinos is always constrained to be ων < 0.005 at 95% c.l.. However, for a sterile neutrino mass of ∼ 0.25eV, ων can be as large as 0.015.
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ar X iv : a st ro - p h / 05 11 50 0 v 3 29 J un 2 00 6 Is cosmology compatible with sterile neutrinos ?
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