THREEFOLD MAXIMAL LEPTON MIXING AND THE SOLAR AND ATMOSPHERIC NEUTRINO DEFICITS

被引:109
作者
HARRISON, PF
PERKINS, DH
SCOTT, WG
机构
[1] UNIV OXFORD, NUCL PHYS LAB, OXFORD OX1 3RH, ENGLAND
[2] RUTHERFORD APPLETON LAB, DIDCOT OX11 0QX, OXON, ENGLAND
关键词
D O I
10.1016/0370-2693(95)00213-5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Threefold maximal mixing would imply a cyclic permutation symmetry among the generations. The data from solar and atmospheric neutrino experiments are consistent with such mixing, and require a hierarchical spectrum of mass-squared differences for the neutrinos. A fit for the two independent mass-squared differences (excluding only the HOMESTAKE solar neutrino result) yields: Delta m(2) = (0.72 +/- 0.18) x 10(-2) eV(2) and Delta m'(2) < 0.9 x 10(-11) eV(2) at 90% confidence, In the case that the neutrino mass spectrum is qualitatively similar to that of the charged leptons and quarks, these results can be re-expressed in terms of the neutrino masses as follows: m(3) similar or equal to 85 +/- 10 meV, and m(1), m(2) < 3 mu eV at 90% confidence. Implications for future experiments are discussed.
引用
收藏
页码:137 / 144
页数:8
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