Solar neutrino puzzle: An oscillation solution with maximal neutrino mixing

被引：227

作者：

Baltz, AJ ^{[1
]}

Goldhaber, AS

Goldhaber, M

机构：

[1] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA

[2] SUNY Stony Brook, Inst Theoret Phys, Stony Brook, NY 11794 USA

来源：

PHYSICAL REVIEW LETTERS | 1998年 / 81卷 / 26期

关键词：

D O I：

10.1103/PhysRevLett.81.5730

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

If, as suggested by the Super-Kamiokande results, nu(mu), and nu(tau) are maximally and "rapidly" (Delta m(2) approximate to 2.2 x 10(-3) eV(2)) mixed, this alone determines the mapping from current to mass eigenstates up to one rotation angle theta mixing nu(e) "more slowly" with a particular, equal-weight combination of nu(mu) and nu(tau). For sin 2 theta = 1, the resulting minimal number of free parameters, yet maximal mixing, shows agreement, with minor modifications, between extant observations of solar neutrinos and predictions by the standard solar model.

引用

页码：5730 / 5733

页数：4

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