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

被引：10

作者：

Tanimoto, M ^{[1
]}

机构：

[1] Ehime Univ, Sci Educ Lab, Matsuyama, Ehime 79077, Japan

来源：

PHYSICAL REVIEW D | 1998年 / 57卷 / 03期

关键词：

D O I：

10.1103/PhysRevD.57.1983

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The three neutrino mass matrices in the SU(5)XU(2) model are studied focusing on neutrino oscillation experiments. The atmospheric neutrino anomaly could be explained by a 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.

引用

页码：1983 / 1986

页数：4

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