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Title: Sterile neutrinos in light of recent cosmological and oscillation data: a multi-flavor scheme approach

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1]; ;  [2];  [3];  [4];  [5]
  1. INFN, Sez. di Roma, Dipartimento di Fisica, Universita di Roma ''La Sapienza'', I-00185 Roma (Italy)
  2. Instituto de Fisica Corpuscular, IFIC, CSIC and Universidad de Valencia (Spain)
  3. Centro de Fisica Teorica de Particulas, Instituto Superior Tecnico, 1049-001 Lisboa (Portugal)
  4. IPPP, Department of Physics, Durham University, Durham DH1 3LE (United Kingdom)
  5. Berkeley Center for Cosmological Physics, Physics Department and Lawrence Berkeley National Laboratory, University of California, Berkeley California 94720 (United States)

Light sterile neutrinos might mix with the active ones and be copiously produced in the early Universe. In the present paper, a detailed multi-flavor analysis of sterile neutrino production is performed. Making some justified approximations allows us to consider not only neutrino interactions with the primeval medium and neutrino coherence breaking effects, but also oscillation effects arising from the presence of three light (mostly-active) neutrino states mixed with two heavier (mostly-sterile) states. First, we emphasize the underlying physics via an analytical description of sterile neutrino abundances that is valid for cases with small mixing between active and sterile neutrinos. Then, we study in detail the phenomenology of (3+2) sterile neutrino models in light of short-baseline oscillation data, including the LSND and MiniBooNE results. Finally, by using the information provided by this analysis, we obtain the expected sterile neutrino cosmological abundances and then contrast them with the most recent available data from Cosmic Microwave Background and Large Scale Structure observations. We conclude that (3+2) models are significantly more disfavored by the internal inconsistencies between sterile neutrino interpretations of appearance and disappearance short-baseline data themselves, rather than by the used cosmological data.

OSTI ID:
22156874
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2009, Issue 01; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

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