Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing

Details Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing

2000-05-16

arxiv.org/abs/hep-ph/0005147v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

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

Scientific paper

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 $\nu_{\mu}$ and $\nu_{\tau}$, is $\simeq \Delta m_{\odot}^2/(2\sqrt{\Delta m_{atm}^2})$. The related topics on Zee-type neutrino mass matrix are also discussed.

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