DESCRIBING ANALYTICALLY THE MSW EFFECT FOR SOLAR NEUTRINOS IN THE PRESENCE OF SOLAR DENSITY PERTURBATIONS

被引:10
作者
ABADA, A
PETCOV, ST
机构
[1] IST NAZL FIS NUCL,I-34014 TRIESTE,ITALY
[2] SCUOLA INT SUPER STUDI AVANZATI,I-34014 TRIESTE,ITALY
关键词
D O I
10.1016/0370-2693(92)91857-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We derive a simple analytic expression for the average probability of two-neutrino matter-enhanced transitions of solar neutrinos in the sun in the case of existence of a thin layer in the interior of the sun in which the density changes much faster (but continuously) than is predicted by the standard solar model.
引用
收藏
页码:153 / 160
页数:8
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