Neutrino magnetic moment solution for the solar neutrino problem and the SNO experiment

被引：0

作者：

Pulido, J ^{[1
]}

机构：

[1] Univ Tecn Lisboa, Ctr Fis Interaccoes, Dept Fis, Inst Super Tecn, P-1049001 Lisbon, Portugal

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2001年 / 100卷

关键词：

D O I：

10.1016/S0920-5632(01)01414-1

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 motivations for the magnetic moment solution to the solar neutrino problem are briefly reviewed and the expected values for a number of observables to be measured by the SNO experiment are calculated assuming three different solar magnetic field profiles. The observables examined are the charged current event rate, the ratio of the neutral current to the charged current event rates and the charged current electron spectrum as well as their first and second moments. The dependence of results on the hep neutrino flux is also analysed and a comparison is made with the corresponding oscillation results.

引用

页码：71 / 73

页数：3

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