SOLAR NEUTRINO OBSERVATIONS AND NEUTRINO OSCILLATIONS

被引：5

作者：

KUO, TK ^{[1
]}

PANTALEONE, J ^{[1
]}

机构：

[1] UNIV CALIF RIVERSIDE,DEPT PHYS,RIVERSIDE,CA 92521

来源：

PHYSICAL REVIEW D | 1990年 / 41卷 / 12期

关键词：

D O I：

10.1103/PhysRevD.41.3842

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The results of recent Kamiokande-II and Cl37 solar-neutrino experiments are quantitatively analyzed assuming the Mikheyev-Smirnov-Wolfenstein solution to the solar-neutrino problem. It is found that the parameter region known as the "large mass" solution to the solar-neutrino problem is disfavored by a little more than 1 f while the "small mass" and "large angle" solutions are in good agreement at this level. The implications on this analysis from time variations in the data are discussed. © 1990 The American Physical Society.

引用

页码：3842 / 3845

页数：4

共 23 条

[1] IS SOLAR NEUTRINO CAPTURE RATE CORRELATED WITH SUNSPOT NUMBER [J].