Bimaximal neutrino mixing and neutrino mass matrix

被引：237

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

[3] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA

来源：

PHYSICAL REVIEW D | 1999年 / 60卷 / 01期

关键词：

D O I：

10.1103/PhysRevD.60.013002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that the bimaximal neutrino mixing pattern suggested by solar and atmospheric neutrino data can be derived from the maximal, symmetric, four-neutrino mixing in the limit that one of the neutrinos is made heavy. imposing the constraints of no neutrinoless double beta decay and a 20% hot dark matter component of the universe leads to the three-neutrino mass matrix recently suggested by Georgi and Glashow. Our result can be useful in constructing theoretical models for the bimaximal pattern. We illustrate this by a simple example. [S0556-2821(99)00713-4].

引用

页数：4

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