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Stringent constraints on cosmological neutrino-antineutrino asymmetries from synchronized flavor transformation

2002/03/31 by Kevork N. Abazajian, J. F. Beacom, John F. Beacom +1 · 11 citations
Physics and Astronomy · #Astrophysics #Astrophysics and Cosmic Phenomena #Big Bang nucleosynthesis #Degeneracy (biology) #Degenerate energy levels #Electron neutrino #Mixing (physics) #Neutrino #Neutrino Physics Research #Neutrino oscillation #Nuclear physics #Nucleosynthesis #Particle physics #Particle physics theoretical and experimental studies #Physics #Pontecorvo–Maki–Nakagawa–Sakata matrix #Quantum mechanics #Solar neutrino #Solar neutrino problem #Stars #astro-ph #hep-ph

paper · pdf · doi:10.1103/physrevd.66.013008

published as Phys.Rev. D66 (2002) 013008 · 11 pages, 6 figures; minor changes to match PRD version

arxiv created 2002/07/17 · openalex publication_date 2002/07/29 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We assess a mechanism which can transform neutrino-antineutrino asymmetries between flavors in the early universe, and confirm that such transformation is unavoidable in the near bimaximal framework emerging for the neutrino mixing matrix. We show that the process is a standard Mikheyev-Smirnov-Wolfenstein flavor transformation dictated by a synchronization of momentum states. We also show that flavor ``equilibration'' is a special feature of maximal mixing, and carefully examine new constraints placed on neutrino asymmetries. In particular, the big bang nucleosynthesis limit on electron neutrino degeneracy |\ensuremathξe|\ensuremath\lesssim0.04 does not apply directly to all flavors, yet confirmation of the large-mixing-angle solution to the solar neutrino problem will eliminate the possibility of degenerate big bang nucleosynthesis.

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