Phenomenology with massive neutrinos

被引:573
作者
Gonzalez-Garcia, M. C. [1 ,2 ]
Maltoni, Michele [3 ,4 ]
机构
[1] SUNY Stony Brook, CN Yang Inst Theoret Phys, Stony Brook, NY 11794 USA
[2] Univ Barcelona, Dept Estructura & Constituents Mat, ICREA, E-08028 Barcelona, Spain
[3] Univ Autonoma Madrid, Fac Ciencias C XI, Dept Fis Teor, E-28049 Madrid, Spain
[4] Univ Autonoma Madrid, Fac Ciencias C XI, Inst Fis Teor, UAM CSIC, E-28049 Madrid, Spain
来源
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2008年 / 460卷 / 1-3期
关键词
D O I
10.1016/j.physrep.2007.12.004
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The current status and some perspectives of the phenomenology of massive neutrinos is reviewed. We start with the phenomenology of neutrino oscillations in vacuum and in matter. We summarize the results of neutrino experiments using solar, atmospheric, reactor and accelerator neutrino beams. We update the leptonic parameters derived from the three-neutrino oscillation interpretation of this data. We describe the method and present results on our understanding of the solar and atmospheric neutrino fluxes by direct extraction from the corresponding neutrino event rates. We present some tests of different forms of new physics which induce new sources of leptonic flavor transitions in vacuum and in matter which can be performed with the present neutrino data. The aim and potential of future neutrino experiments and facilities to further advance in these fronts is also briefly summarized. Last, the implications of the LSND observations are discussed, and the status of extended models which could accommodate all flavor-mixing signals is presented in the light of the recent results from MiniBooNE. (c) 2008 Elsevier B.V All rights reserved.
引用
收藏
页码:1 / 129
页数:129
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