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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
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BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20181028T010000
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BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20181112T143000
DTEND;TZID=Europe/Rome:20181112T163000
DTSTAMP:20260912T102617
CREATED:20181106T184755Z
LAST-MODIFIED:20181119T184734Z
UID:13714-1542033000-1542040200@w3.lnf.infn.it
SUMMARY:From simplified to gauge invariant realizations of light pseudoscalar  portal
DESCRIPTION:WIMPs mostly interacting with the SM states through a pseudoscalar mediator can achieve the correct relic density evading current constraints from Dark Matter Direct Detection. I will discuss some realistic implementation for a dark pseudoscalar portal with particular focus to the prospects for Direct Detection at next future facilities.
URL:/event/from-simplified-to-gauge-invariant-realizations-of-light-pseudoscalar-portal/
LOCATION:Aula Seminari\, Via Enrico Fermi\, 40\, Frascati\, Roma\, 00044\, Italia
CATEGORIES:Seminari teorici
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