KAMIOKANDE SOLAR-NEUTRINO RESULTS

被引：108

作者：

SUZUKI, Y ^{[1
]}

机构：

[1] UNIV TOKYO,INST COSM RAY RES,TANASHI,TOKYO 188,JAPAN

来源：

NUCLEAR PHYSICS B | 1995年

关键词：

D O I：

10.1016/0920-5632(94)00733-C

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The results on the solar neutrino measurement covering over 7 years in the Kaminokande detector are explained, and their systematic errors are briefly reviewed. The time averaged flux assuming the shape of the B-8 beta decay is (2.89(-0.21)(+0.22)+/-0.35) x 10(6) cm(2)/sec and the ratio of the flux to the standard solar model of Bahcall and Pinsonnault is 0.51 +/- 0.04 +/- 0.06. Model independent approaches to the solar neutrino problem that we can conduct by the future solar neutrino experiment, Superkamiokande, are also presented.

引用

页码：54 / 59

页数：6