Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing

2000/05/16 by M. Matsuda, Matsuda, M., C. Jarlskog +5
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/0005147

5 pages, no figure, Talk given by M. Matsuda at Workshop on Neutrino Oscillations and their Origin, Fuji-Yoshida, Japan, 11-13 Feb 2000

arxiv created 2000/05/16 · arxiv updated 2009/11/30

Abstract

It is shown that the bi-maximal solution is the only possibility to reconcile Zee-type neutrino mass matrix with three flavors to the current atmospheric and solar neutrino experimental data. The mass of the lightest neutrino, which consist mostly of ν_μ and ν_τ, is ≃ Δm_\odot²/(2√Δm_atm²). The related topics on Zee-type neutrino mass matrix are also discussed.

Related

• Zee model and Neutrinoless double beta decay
• Constraining Neutrino Mass Matrix from Modified BM with Softly Broken μ-τ Symmetry
• Models of maximal atmospheric neutrino mixing
• Large Neutrino Flavor Mixings and Lepton Mass Matrices
• Neutrino Mass Matrix a la Mode