Cosmological constraints on a light nonthermal sterile neutrino
- Dipartimento di Fisica Teorica, Universita di Torino, Via P. Giuria 1, I-10125 Torino (Italy) and INFN, Sezione di Torino, Via P. Giuria 1, I-10125 Torino (Italy) and Laboratoire d'Annecy-le-Vieux de Physique Thorique LAPTH, Universite de Savoie, CNRS/IN2P3, 74941 Annecy-le-vieux (France)
- PH-TH, CERN-CH-1211 Geneva 23 (Switzerland)
Although the MiniBooNE experiment has severely restricted the possible existence of light sterile neutrinos, a few anomalies persist in oscillation data, and the possibility of extra light species contributing as a subdominant hot (or warm) component is still interesting. In many models, this species would be in thermal equilibrium in the early universe and share the same temperature as active neutrinos, but this is not necessarily the case. In this work, we fit up-to-date cosmological data with an extended {lambda}CDM model, including light relics with a mass typically in the range 0.1-10 eV. We provide, first, some nearly model-independent constraints on their current density and velocity dispersion, and second, some constraints on their mass, assuming that they consist either in early decoupled thermal relics, or in nonresonantly produced sterile neutrinos. Our results can be used for constraining most particle-physics-motivated models with three active neutrinos and one extra light species. For instance, we find that at the 3{sigma} confidence level, a sterile neutrino with mass m{sub s}=2 eV can be accommodated with the data provided that it is thermally distributed with T{sub s}/T{sub {nu}}{sup id} < or approx. 0.8 or nonresonantly produced with {delta}N{sub eff} < or approx. 0.5. The bounds become dramatically tighter when the mass increases. For m{sub s} < or approx. 0.9 eV and at the same confidence level, the data is still compatible with a standard thermalized neutrino.
- OSTI ID:
- 21266337
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 79, Issue 4; Other Information: DOI: 10.1103/PhysRevD.79.045026; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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