NON-DYNAMIC CONTRIBUTIONS TO LEFT RIGHT TRANSITIONS IN THE SOLAR NEUTRINO PROBLEM

被引：53

作者：

VIDAL, J ^{[1
]}

WUDKA, J ^{[1
]}

机构：

[1] UNIV VALENCIA,CSIC,INST FIS INVEST CIENCIAS,BURJASSOT,SPAIN

来源：

PHYSICS LETTERS B | 1990年 / 249卷 / 3-4期

关键词：

D O I：

10.1016/0370-2693(90)91019-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The conditions under which the adiabatic phases can produce a reduction in the solar neutrino flux are studied for a realistic model of the solar magnetic field. Within the adiabatic approximation, it is found that μ > 10-13 μBohr will produce a sensible decrease in the flux. The possible correlations with the solar cycle, as well as the corrections to the adiabatic approximation are briefly considered. © 1990.

引用

页码：473 / 477

页数：5

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