Gauge model for maximal neutrino mixing

被引:97
作者
Mohapatra, RN [1 ]
Nussinov, S
机构
[1] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[2] Tel Aviv Univ, Dept Phys, IL-69978 Tel Aviv, Israel
基金
美国国家科学基金会;
关键词
D O I
10.1016/S0370-2693(98)01169-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The recently announced Super-Kamiokande data on atmospheric neutrino oscillation seems to require a maximal mixing between the nu(mu) and nu(tau) within the conventional three neutrino picture. It is then tempting to suggest as has been done in literature, that the solar neutrino deficit be also understood as resulting from a maximal mixing between nu(e) and nu(mu). In this letter, we propose a left-right symmetric extension of the standard model where permutation symmetry leads to one of the maximal mixing patterns in a technically natural manner. The double seesaw mechanism gives small Majorana masses for neutrinos needed to understand the atmospheric as well as the solar neutrino puzzles. (C) 1998 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:299 / 304
页数:6
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