Massive neutrinos and lepton-flavour-violating processes

Details Massive neutrinos and lepton-flavour-violating processes Massive neutrinos and lepton-flavour-violating processes

2001-09-18

arxiv.org/abs/hep-ph/0109161v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, 3 figures, Talk given at Cairo International Conference on High Energy Physics, Cairo (CICHEP 2001), Egypt, 9-14, Ja

Scientific paper

If neutrino masses and mixings are suitable to explain the atmospheric and solar neutrino fluxes, this amounts to contributions to FCNC processes, in particular $\mu\to e, \gamma$. If the theory is supersymmetric and the origin of the masses is a see-saw mechanism, we show that the prediction for BR($\mu\to e, \gamma$) is in general larger than the experimental upper bound, especially if the solar data are explained by a large angle MSW effect, which recent analyses suggest as the preferred scenario.

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