Finally neutrino has mass
arXiv:hep-ph/9902462 · doi:10.1142/S0217751X00000318
Abstract
The present status of the problem of neutrino mass, mixing and neutrino oscillations is briefly summarized. The evidence for oscillations of atmospheric neutrinos found recently in the Super-Kamiokande experiment is discussed. Indications in favor of neutrino oscillations obtained in solar neutrino experiments and in the accelerator LSND experiment are also considered. Implications of existing neutrino oscillation data for neutrino masses and mixing are discussed.
27 pages. Final version to be published in Int. J. Mod. Phys. A
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Cited by in corpus (6)
- Neutrinos in cosmology
- Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino
- Complementary Ansatz for the neutrino mass matrix
- Implications of texture 4 zero lepton mass matrices for U_{e3}
- Optimization of the design of OMNIS, the observatory of multiflavor neutrinos from supernovae
- The massive neutrino-like particle of the non-linear electromagnetic field theory