Lepton flavor mixing in the Wolfenstein scheme

被引:2
|
作者
Gupta, V. [1 ]
Sanchez-Colon, G. [1 ]
Rajpoot, S. [2 ]
Wang, H. -C. [2 ]
机构
[1] IPN, Dept Fis Aplicada, Ctr Invest & Estudios Avanzados, Unidad Merida, Merida 97310, Yucatan, Mexico
[2] Calif State Univ Long Beach, Dept Phys & Astron, Long Beach, CA 90840 USA
来源
PHYSICAL REVIEW D | 2013年 / 87卷 / 07期
关键词
NEUTRINO MASS; SEARCH; MODEL;
D O I
10.1103/PhysRevD.87.073009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We mimic the Wolfenstein scheme of quark flavor mixing to describe neutrino oscillations in the standard model. We identify the parameter lambda with the experimentally measured value of the mixing element responsible for atmospheric neutrino oscillations. The matrix elements responsible for solar neutrino oscillations and the Chooz angle are taken to be proportional to lambda(2) and lambda(3), respectively. Using present world average data on neutrinos, we derive bounds on the other parameters, A, rho, and eta of the new scheme. DOI: 10.1103/PhysRevD.87.073009
引用
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页数:4
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