Neutrino mass matrix with U(2) flavor symmetry and neutrino oscillations

Details Neutrino mass matrix with U(2) flavor symmetry and neutrino oscillations Neutrino mass matrix with U(2) flavor symmetry and neutrino oscillations

1997-06-25

arxiv.org/abs/hep-ph/9706497v2

Phys.Rev.D57:1983-1986,1998

Physics

High Energy Physics

High Energy Physics - Phenomenology

12 pages, LaTex file, to be published in PRD

Scientific paper

10.1103/PhysRevD.57.1983

The three neutrino mass matrices in the $SU(5)\times U(2)$ model are studied focusing on the neutrino oscillation experiments. The atmospheric neutrino anomaly could be explained by the large $\nu_{\mu} - \nu_{\tau}$ oscillation. The long baseline experiments are expected to detect signatures of the neutrino oscillation even if the atmospheric neutrino anomaly is not due to the neutrino oscillation. However, the model cannot solve the solar neutrino deficit while it could be reconciled with the LSND data.

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