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VERSION:2.0
PRODID:-//CERN//INDICO//EN
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SUMMARY:OSCILLATING NEUTRINOS AND MU --> E\, GAMMA
DTSTART;VALUE=DATE-TIME:20001123T113000Z
DTEND;VALUE=DATE-TIME:20001123T123000Z
DTSTAMP;VALUE=DATE-TIME:20261012T092134Z
UID:indico-event-1198@indico.ific.uv.es
DESCRIPTION:If neutrino masses and mixings are suitable to explain the atm
 ospheric and solar neutrino fluxes\, this amounts to contributions to FCNC
  processes\, in particular $\\mu\\rightarrow e\, \\gamma$. If the theory i
 s supersymmetric and the origin of the masses is a see-saw mechanism\, the
  predictions for BR($\\mu\\rightarrow e\, \\gamma$) naturally exceed the e
 xperimental bounds.\n\nhttps://indico.ific.uv.es/event/1198/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1198/
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