Four-Neutrino Oscillations
V. Barger
Abstract
Models with three active neutrinos and one sterile neutrino can naturally account for maximal oscillations of atmospheric neutrinos, explain the solar neutrino deficit, and accommodate the results of the LSND experiment. The models predict either νeντ or νeνs oscillations in long-baseline experiments with the atmospheric δm2 scale and amplitude determined by the LSND oscillations.
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