Neutrino anomalies in an extended Zee model

被引:52
作者
Joshipura, AS [1 ]
Rindani, SD [1 ]
机构
[1] Phys Res Lab, Theoret Phys Grp, Ahmadabad 380009, Gujarat, India
关键词
D O I
10.1016/S0370-2693(99)00995-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss an extended SU(2) x U(1) model which naturally leads to mass scales and mixing angles relevant for understanding both the solar and atmospheric neutrino anomalies. No right-handed neutrinos are introduced in the model. The model uses a softly broken L-e - L-mu - L-T symmetry. Neutrino masses arise only at the loop level. The one-loop neutrino masses which arise as in the Zee model solve the atmospheric neutrino anomaly while breaking of L-e - L-mu - L-T generates at two-loop order a mass splitting needed for the vacuum solution of the solar neutrino problem. A somewhat different model is possible which accommodates the large-angle MSW resolution of the solar neutrino problem. (C) 1999 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:239 / 243
页数:5
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