The scheme of mixing of three neutrinos with a mass hierarchy is considered for the explanation of the solar and atmospheric neutrino problems through neutrino oscillations. It is shown that the recent results of the CHOOZ experiment imply that the element U_{e3} of the neutrino mixing matrix is small, that the oscillations of solar neutrinos are described by the two-generation formalism and that the oscillations of solar and atmospheric neutrinos decouple. Furthermore, if |U_{e3}|<<1 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 neutrin...
We present an analysis of the neutrino oscillation solutions of the solar and atmospheric neutrino p...
The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the...
Various solutions of the atmospheric neutrino data are reviewed. Apart from orthodox two flavor $\nu...
We perform a global three generation analysis of the current solar and atmospheric evidence in favor...
We perform a global three generation analysis of the current solar and atmospheric evidence in favor...
Results of a new analysis of the CHOOZ data, performed in the framework of three-neutrino mixing, ar...
We investigate the three-neutrino mixing scheme for solving the atmospheric and LSND anomalies. We f...
We analyze the atmospheric neutrino data in the context of three flavor neutrino oscillations taking...
We have analyzed the results of reactor and accelerator neutrino oscillation experiments in the fram...
We perform a phenomenological analysis of neutrino oscillation in a four generation framework introd...
The three neutrino Zee model and its extension, including three active and one sterile species, are ...
We present a systematic analysis of the three-flavor Mikheyev-Smirnov-Wolfenstein (MSW) oscillation ...
The interpretation of the existing experimental evidences for oscillations of neutrinos in schemes w...
We present a formalism for the description of oscillations in matter of solar, atmospheric and long-...
We analyze the evidence for solar and atmospheric neutrino oscillations in a common three-flavor osc...
We present an analysis of the neutrino oscillation solutions of the solar and atmospheric neutrino p...
The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the...
Various solutions of the atmospheric neutrino data are reviewed. Apart from orthodox two flavor $\nu...
We perform a global three generation analysis of the current solar and atmospheric evidence in favor...
We perform a global three generation analysis of the current solar and atmospheric evidence in favor...
Results of a new analysis of the CHOOZ data, performed in the framework of three-neutrino mixing, ar...
We investigate the three-neutrino mixing scheme for solving the atmospheric and LSND anomalies. We f...
We analyze the atmospheric neutrino data in the context of three flavor neutrino oscillations taking...
We have analyzed the results of reactor and accelerator neutrino oscillation experiments in the fram...
We perform a phenomenological analysis of neutrino oscillation in a four generation framework introd...
The three neutrino Zee model and its extension, including three active and one sterile species, are ...
We present a systematic analysis of the three-flavor Mikheyev-Smirnov-Wolfenstein (MSW) oscillation ...
The interpretation of the existing experimental evidences for oscillations of neutrinos in schemes w...
We present a formalism for the description of oscillations in matter of solar, atmospheric and long-...
We analyze the evidence for solar and atmospheric neutrino oscillations in a common three-flavor osc...
We present an analysis of the neutrino oscillation solutions of the solar and atmospheric neutrino p...
The Sun is a source of high energy neutrinos (E > 10 GeV) produced by cosmic ray interactions in the...
Various solutions of the atmospheric neutrino data are reviewed. Apart from orthodox two flavor $\nu...