Bimaximal neutrino mixings from lopsided mass matrices

被引：53

作者：

Babu, KS ^{[1
]}

Barr, SM

机构：

[1] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA

[2] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA

来源：

PHYSICS LETTERS B | 2002年 / 525卷 / 3-4期

关键词：

D O I：

10.1016/S0370-2693(01)01455-1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Current solar and atmospheric neutrino oscillation data seem to favor a bimaximal pattern for neutrino mixings where the matrix elements U-e2 and U-mu3 are of order one, while U-e3 is much smaller. We show that such a pattern can be obtained quite easily in theories with "lopsided" mass matrices for the charged leptons and the down type quarks. A relation connecting the solar and atmospheric neutrino mixing angles is derived, tan(2)theta(atm) similar or equal to 1 + tan(2)theta(sol), which predicts sin(2)2theta(atm) similar or equal to 0.97 corresponding to the best fit LMA solution for solar neutrinos. Predictive schemes in SO(10) realizing these ideas are presented. A new class of SO(10) models with lopsided mass matrices is found which makes use of an adjoint VEV along the I-3R direction, rather than the traditional B - L direction. (C) 2002 Elsevier Science B.V. All rights reserved.

引用

页码：289 / 296

页数：8

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