BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//INFN-LNF - ECPv5.14.2.1//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:INFN-LNF
X-ORIGINAL-URL:https://w3.lnf.infn.it
X-WR-CALDESC:Eventi per INFN-LNF
BEGIN:VTIMEZONE
TZID:Europe/Rome
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20180325T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20181028T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20181205T143000
DTEND;TZID=Europe/Rome:20181205T163000
DTSTAMP:20260911T033155
CREATED:20181022T184820Z
LAST-MODIFIED:20181212T184719Z
UID:13579-1544020200-1544027400@w3.lnf.infn.it
SUMMARY:Neutrino Lines from Dark Matter
DESCRIPTION:While photon lines – or monochromatic photons-are known to arise in many dark matter models\,  neutrino lines are not so common.\nIn this talk\, I will discuss simple dark matter models\, whose main indirect detection signature is the production of monochromatic neutrinos.  Such features play an important role in indirect dark matter searches because they can be better discriminated against the astrophysical background.\nIn the first part of my talk\, I will discuss decaying dark matter. In particular\, I will focus on  singlet majorons\, which naturally produce neutrino lines. Then\, in the second part\,I will briefly describe the properties that simple models must have in order to produce\, in the near future\,an observable flux of neutrino lines from dark matter annihilations. In both parts\, I will  discuss the implications  for neutrino telescopes and the interplay with other indirect detection channels.
URL:/event/neutrino-lines-from-dark-matter/
LOCATION:Aula Salvini
CATEGORIES:Seminari teorici
END:VEVENT
END:VCALENDAR