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VERSION:2.0
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SUMMARY:Radiative neutrinos and dark matter
DTSTART;VALUE=DATE-TIME:20150226T150000Z
DTEND;VALUE=DATE-TIME:20150226T160000Z
DTSTAMP;VALUE=DATE-TIME:20261012T112312Z
UID:indico-event-2440@indico.ific.uv.es
DESCRIPTION:Radiative generations of neutrino masses are alternative to se
 esaw mechanism and testable at LHC.\nIn this talk I'd like to introduce to
  a radiative neutrino mass model\, Zee-Babu mechanism\, and extend it to i
 ncorporate dark matter candidate. Especially\, I'll show that this model c
 an explain the 3.5 keV X-ray line signal.\n\nhttps://indico.ific.uv.es/eve
 nt/2440/
LOCATION:Campus Burjassot 4-4-4426 - Seminari Física Teòrica
URL:https://indico.ific.uv.es/event/2440/
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