Atmospheric Neutrino Oscillation and a Phenomenological Lepton Mass Matrix

Details Atmospheric Neutrino Oscillation and a Phenomenological Lepton Mass Matrix Atmospheric Neutrino Oscillation and a Phenomenological Lepton Mass Matrix

1997-09-18

arxiv.org/abs/hep-ph/9709388v2

Phys.Rev. D57 (1998) 4429-4432

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, Latex file, small corrections in text and references, to appear in PRD

Scientific paper

10.1103/PhysRevD.57.4429

We propose simple phenomenological lepton mass matrices which describe the three neutrinos almost degenerate in mass, leading to a very large mixing angle between $\nu_\mu$ and $\nu_\tau$, as consistent with a recent report on atmospheric neutrino oscillation from the Superkamiokande collaboration. Our matrix model also gives $\nu_e-\nu_\mu$ mixing in agreement with the value required for neutrino oscillation to explain the solar neutrino problem.

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