Abstract

We have considered the results of solar and atmospheric neutrino oscillation experiments in the scheme of mixing of three neutrinos with a mass hierarchy. It is shown that (if m 3 2−m 1 2>10 −3 eV 2 ) the recent results of the CHOOZ experiment imply that | U e3 | 2≪1 ( U is the neutrino mixing matrix), that the oscillations of solar neutrinos are described by the two-generation formalism and that the oscillations of solar and atmospheric neutrinos decouple. It is also shown that if not only | U e3 | 2≪1 but also | U e3 |≪1, then the oscillations of atmospheric neutrinos do not depend on matter effects and are described by the two-generation formalism. In this case, with an appropriate identification of the mixing parameters, the two-generation analyses of solar and atmospheric neutrino data provide direct information on the mixing parameters of three neutrinos. We discuss the possibility to get information on | U e3 | 2 in long-baseline neutrino oscillation experiments.

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