Zee-type Neutrino Mass Matrix and Bi-Maximal Mixing

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dc.creatorMatsuda, M.
dc.creatorJarlskog, C.
dc.creatorSkadhauge, S.
dc.creatorTanimoto, M.
dc.date2000-05-16
dc.date.accessioned2026-07-07T03:41:28Z
dc.date.available2026-07-07T03:41:28Z
dc.descriptionIt 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.
dc.description5 pages, no figure, Talk given by M. Matsuda at Workshop on Neutrino Oscillations and their Origin, Fuji-Yoshida, Japan, 11-13 Feb 2000
dc.identifierhttps://arxiv.org/abs/hep-ph/0005147
dc.identifierhttp://arxiv.org/abs/hep-ph/0005147
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39597
dc.subjectHigh Energy Physics - Phenomenology
dc.titleZee-type Neutrino Mass Matrix and Bi-Maximal Mixing
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