Finally neutrino has mass
S.M. Bilenky, C. Giunti, C.W. Kim

TL;DR
This paper reviews the current evidence for neutrino mass and oscillations, discussing experimental results from Super-Kamiokande, solar neutrino, and LSND experiments, and explores their implications for neutrino properties.
Contribution
It provides a comprehensive summary of recent experimental findings on neutrino oscillations and discusses their implications for neutrino mass and mixing models.
Findings
Super-Kamiokande confirmed atmospheric neutrino oscillations
Solar neutrino experiments suggest neutrino flavor change
LSND experiment indicates possible neutrino oscillations beyond three flavors
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.
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