Theoretical interpretation of recent neutrino oscillation data

Physics

Scientific paper

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Neutrino Mass And Mixing, Solar Neutrinos, Particle Emission, Solar Wind

Scientific paper

The theoretical interpretation of the current neutrino phenomenology is reviewed, in the context of three and four neutrino mixing. We discuss the status of atmospheric vμ oscillations and the recent indications from the KEK-to-Kamioka (K2K) experiment. We also review the status of solar ve oscillations after the Sudbury Neutrino Observatory (SNO) measurements. The three-neutrino mixing scenario emerges as a consistent theoretical interpretation of solar, atmospheric, and reactor data. Conversely, the inclusion of LSND accelerator data in an extended four-neutrino scenario generates a ``tension'' between data subsets in global fits. We also comment about the role of possible new neutrino interactions.

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