arXiv · hep-ph/0005147
Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing
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 $\simeq Δm_{\odot}^2/(2\sqrt{Δm_{atm}^2})$. The related topics on Zee-type neutrino mass matrix are also discussed.
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M. Matsuda, C. Jarlskog, S. Skadhauge, M. Tanimoto. 2000-05-16. Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing. https://arxiv.org/abs/hep-ph/0005147
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