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SUMMARY:#StudentSeminar: Asymmetric Dark Matter
DTSTART;VALUE=DATE-TIME:20250918T090000Z
DTEND;VALUE=DATE-TIME:20250918T103000Z
DTSTAMP;VALUE=DATE-TIME:20260810T053608Z
UID:indico-event-8228@indico.ific.uv.es
DESCRIPTION:Although the Standard Model (SM) has been remarkably successfu
 l\, several theoretical and phenomenological challenges remain unresolved.
  A major issue is the absence of a viable dark matter (DM) candidate\, des
 pite strong indirect evidence for its existence from galactic and cluster-
 scale observations. Another open question is the observed matter–antimat
 ter asymmetry: while the SM can generate such an asymmetry\, the predicted
  amount falls short of observations. Asymmetric dark matter provides a com
 pelling framework to address both problems simultaneously\, particularly g
 iven that observations indicate the DM abundance is only about five times 
 larger than that of ordinary matter. In this work\, we propose a supersymm
 etric model that naturally accommodates this mechanism.\n\nhttps://indico.
 ific.uv.es/event/8228/
LOCATION:Universe 1001-Primera-1-1-1 - Paterna. Seminario
URL:https://indico.ific.uv.es/event/8228/
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