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SUMMARY:Constraining Secluded Dark Matter Scenarios with HAWC
DTSTART;VALUE=DATE-TIME:20191113T071000Z
DTEND;VALUE=DATE-TIME:20191113T073000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182841Z
UID:indico-contribution-1558@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Sergio Hernandez Cadena (Instituto de Física\, UNAM
 )\nIt is possible that DM particles are secluded to their own dark sector\
 , where the interactions are carried by one or several dark mediators. If 
 this dark sector exists\, DM particles do not couple directly to the stand
 ard model (SM) particles\, as in the case of WIMP scenarios. However\, ind
 irect DM searches are still possible if we assume that dark mediators are 
 coupled to SM particles through a kinetic mixing parameter. The HAWC Obser
 vatory is a wide-field-of-view gamma-ray experiment with a high duty cycle
  (>95%) and looking for gamma rays with energies between 1 and 100 TeV. So
 \,  for secluded DM candidates in the TeV range\, the HAWC Observatory is 
 able to explore and constrain the parameter space of dark sector scenarios
  by searching for gamma-ray signals of dark mediator decays in nearby astr
 ophysical targets. Here\, we present preliminary results of these indirect
  searches using HAWC data.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/
 contributions/1558/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1558/
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