ANTINEUTRINOS FROM THE SUN

被引：24

作者：

AKHMEDOV, EK

机构：

[1] Kurchatov Institute of Atomic Energy

来源：

PHYSICS LETTERS B | 1991年 / 255卷 / 01期

关键词：

D O I：

10.1016/0370-2693(91)91143-J

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Various mechanisms are discussed by which the sun could emit electron antineutrinos nu-BAR e in addition to neutrinos nu-e, special attention being paid to the neutrino oscillations + spin-flavor precession scenario. For the latter, the probabilities of nu-e --> nu-BAR e conversion in the sun are calculated and experimental consequences are discussed. It is shown that this scenario can be distinguished from other nu-BAR e-producing mechanisms by its unique prediction of time variations of the nu-BAR e flux in direct correlation with solar activity, and also due to different consequences for experiments based on neutral-current mediated reactions.

引用

页码：84 / 88

页数：5

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