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Large neutrino asymmetries from neutrino oscillations

R. Foot, M. J. Thomson, and R. R. Volkas
Phys. Rev. D 53, R5349(R) – Published 15 May 1996
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Abstract

We reexamine neutrino oscillations in the early universe. Contrary to previous studies, we show that large neutrino asymmetries can arise due to oscillations between ordinary neutrinos and sterile neutrinos. This means that the big bang nucleosynthesis (BBN) bounds on the mass and mixing of ordinary neutrinos with sterile neutrinos can be evaded. Also, it is possible that the neutrino asymmetries can be large enough (≳10%) to have a significant effect on BBN through nuclear reaction rates.

  • Received 14 September 1995

DOI:https://doi.org/10.1103/PhysRevD.53.R5349

©1996 American Physical Society

Authors & Affiliations

R. Foot, M. J. Thomson, and R. R. Volkas

  • Research Centre for High Energy Physics, School of Physics, University of Melbourne, Parkville, 3052 Australia

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Issue

Vol. 53, Iss. 10 — 15 May 1996

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