Neutrino masses and bimaximal mixing

M. Jezabek, Y. Sumino

Research output: Contribution to journalArticlepeer-review

68 Citations (Scopus)


Solar and atmospheric neutrino anomalies are described by bimaximal mixing of three Majorana neutrinos. Neutrino oscillations in appearance ve ⇌ vμ,vτ and in disappearance ve long baseline and atmospheric experiments are sensitive to deviations from the ideal bi maxi mal mixing. It is suggested that these deviations may be dominated by a rotation in the electron-muon plane of the generation space. Simple seesaw models are described supporting this idea. The rotation angle is estimated from Fritzsch' s relation. Predictions are presented for oscillations in long baseline experiments, for solar neutrinos, and for the rates of neutrinoless double beta decays.

Original languageEnglish
Pages (from-to)139-146
Number of pages8
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Issue number1-3
Publication statusPublished - 1999

ASJC Scopus subject areas

  • Nuclear and High Energy Physics


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