Four-way neutrino oscillations

被引:98
作者
Barger, V
Weiler, TJ
Whisnant, K
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[2] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA
[3] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA
关键词
D O I
10.1016/S0370-2693(98)00325-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a four-neutrino model with three active neutrinos and one sterile neutrino which naturally has maximal nu(mu)-->nu(tau) oscillations of atmospheric neutrinos and can explain the solar neutrino and LSND results. The model predicts nu(e)-->nu(tau) and nu(e)-->nu(mu) oscillations in long-baseline experiments with L/E much greater than 1 km/GeV with amplitudes that are determined by the LSND oscillation amplitude and argument controlled by the atmospheric delta m(2). (C) 1998 Published by Elsevier Science B.V. All rights reserved.
引用
收藏
页码:97 / 104
页数:8
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