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:20190331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20191027T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20190624T110000
DTEND;TZID=Europe/Rome:20190624T123000
DTSTAMP:20260901T051546
CREATED:20190607T184717Z
LAST-MODIFIED:20190701T184825Z
UID:19508-1561374000-1561379400@w3.lnf.infn.it
SUMMARY:Model independent analysis of MeV scale dark matter
DESCRIPTION:Recent results from several direct detection experiments have imposed severe constraints on the multi-GeV mass window for various dark mat- ter(DM) models. However\, many of these experiments are not sensitive to MeV scale DM as the corresponding recoil energies are much below the detector thresholds. In this regard\, we reexamined the light scalar DM in a model-independent approach in our recent work. For such a DM\, it should not be assumed that it annihilates into a pair of free quarks. Instead\, it becomes necessary to determine the effective couplings of DM to hadrons and calculate the annihilation rate with hadrons in final states. In this talk\, I will discuss the methodology for determining this effective coupling along with various constraints coming from cosmological and astrophysical observations.
URL:/event/model-independent-analysis-of-mev-scale-dark-matter/
LOCATION:Aula Salvini
CATEGORIES:Seminari teorici
END:VEVENT
END:VCALENDAR