A NEUTRINO DECAY MODEL, SOLAR ANTINEUTRINOS AND ATMOSPHERIC NEUTRINOS

被引：68

作者：

ACKER, A ^{[1
]}

JOSHIPURA, A ^{[1
]}

PAKVASA, S ^{[1
]}

机构：

[1] PHYS RES LAB,AHMEDABAD 380009,GUJARAT,INDIA

来源：

PHYSICS LETTERS B | 1992年 / 285卷 / 04期

关键词：

D O I：

10.1016/0370-2693(92)91520-J

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The neutrino decay solution to the solar neutrino problem calls for large mixing and a short lifetime for the decaying neutrino. We propose a model for neutrino masses which has these features and furthermore leads to decays into antineutrinos. The resulting fluxes of v(e)'sBAR are detectable in future solar neutrino detectors. The large v(e)-v(mu) mixing can account for the atmospheric neutrino anomaly at the same time.

引用

页码：371 / 375

页数：5

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