NEUTRINO TRANSITIONAL MAGNETIC-MOMENT AND NON-ABELIAN DISCRETE SYMMETRY

被引：21

作者：

CHANG, D

KEUNG, WY

SENJANOVIC, G

机构：

[1] FERMI NATL ACCELERATOR LAB, BATAVIA, IL 60510 USA

[2] UNIV ILLINOIS, DEPT PHYS, CHICAGO, IL 60680 USA

[3] UNIV ZAGREB, DEPT THEORET PHYS, YU-41001 Zagreb, YUGOSLAVIA

[4] UNIV DELAWARE, BARTOL RES INST, NEWARK, DE 19711 USA

来源：

PHYSICAL REVIEW D | 1990年 / 42卷 / 05期

关键词：

D O I：

10.1103/PhysRevD.42.1599

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We propose a mechanism which naturally will give rise to a small mass but a large transitional magnetic moment for the neutrino such that the solar-neutrino deficit problem can be explained. The idea is a discrete version of Voloshin's SU(2) mechanism. An example of such a mechanism using the quaternion group is illustrated. © 1990 The American Physical Society.

引用

页码：1599 / 1603

页数：5

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