Solar models and solar neutrino oscillations

被引：141

作者：

Bahcall, JN ^{[1
]}

Peña-Garay, C ^{[1
]}

机构：

[1] Inst Adv Study, Sch Nat Sci, Princeton, NJ 08540 USA

来源：

NEW JOURNAL OF PHYSICS | 2004年 / 6卷

基金：

美国国家科学基金会;

关键词：

D O I：

10.1088/1367-2630/6/1/063

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We provide a summary of the current knowledge, theoretical and experimental, of solar neutrino fluxes and of the masses and mixing angles that characterize solar neutrino oscillations. We also summarize the principal reasons for performing new solar neutrino experiments and what we anticipate from future studies.

引用

页码：1 / 19

页数：19

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