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Atmospheric and Solar neutrinos in the light of the SuperKamiokande results

1999/01/07 by Riccardo Barbieri, Barbieri, Riccardo
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Particle physics theoretical and experimental studies #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/9901241

8 pages, lecture at Erice 98

arxiv created 1999/01/07 · openalex publication_date 1999/01/07 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The hierarchy Δm2atm ≫ Δm2_\odot and the large θ23 mixing angle, as suggested by neutrino oscillation experiments, can be accounted for by a variety of lepton flavour models. A dichotomy emerges: i) Models were all neutrino masses are bounded by matm≡ (Δm2atm)1/2≈ 0.03 eV; ii) Models of quasi-degenerate neutrinos. It is shown how these different patterns of neutrino masses may arise from different lepton flavour symmetries. Physical implications are discussed in the various cases.

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