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SUMMARY:Cosmology and Signals of Light Dark Matter - Mariana Carrillo-Gonz
 ález (ICL)
DTSTART:20211122T130000Z
DTEND:20211122T140000Z
UID:TALK163009@talks.cam.ac.uk
CONTACT:James Bonifacio
DESCRIPTION:Strong bounds from CMB observations have pushed us away from t
 he standard WIMP picture of dark matter (DM). Nevertheless\, a dark matter
  candidate of thermal origin does not require elastic weak interactions to
  lead to the observed DM abundance. In fact\, the simple appearance of Maj
 orana masses changes the standard picture of WIMP DM.  In this talk\, I wi
 ll present a careful analysis of the cosmological evolution of light pseud
 o-Dirac DM. I will focus on the importance of carefully computing the DM a
 bundance to understand the DM signals (such as the Xenon1T excess) and on 
 the complementarity of different searches. 
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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