Neutrino Anomalies in an Extended Zee Model

Details Neutrino Anomalies in an Extended Zee Model Neutrino Anomalies in an Extended Zee Model

1999-07-16

arxiv.org/abs/hep-ph/9907390v2

Phys.Lett. B464 (1999) 239-243

Physics

High Energy Physics

High Energy Physics - Phenomenology

11 pages including 2 figures; a reference added and text changed accordingly

Scientific paper

10.1016/S0370-2693(99)00995-8

We discuss an extended $SU(2)\times U(1)$ model which naturally leads to mass scales and mixing angles relevant for understanding both the solar and atmospheric neutrino anomalies. No right-handed neutrinos are introduced in the model.The model uses a softly broken $L_e-L_{\mu}-L_{\tau}$ symmetry. Neutrino masses arise only at the loop level. The one-loop neutrino masses which arise as in the Zee model solve the atmospheric neutrino anomaly while breaking of $L_e-L_{\mu}-L_{\tau}$ generates at two-loop order a mass splitting needed for the vacuum solution of the solar neutrino problem. A somewhat different model is possible which accommodates the large-angle MSW resolution of the solar neutrino problem.

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