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SUMMARY:Current and Future WIMP Searches with Fermi-LAT\, HAWC\, and SWGO
DTSTART;VALUE=DATE-TIME:20191113T030000Z
DTEND;VALUE=DATE-TIME:20191113T033000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182831Z
UID:indico-contribution-1523@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Andrea Albert (Los Alamos National Lab)\nEvidence su
 ggests ~85% of the mass in the Universe is dark matter (DM). Several promi
 sing DM theories predict that it is a fundamental particle. The most famou
 s of which is the Weakly Interacting Massive Particle (WIMP). WIMPs that a
 nnihilate at a weak-scale cross section that were in thermal equilibrium i
 n the Universe produce the observed DM abundance today. DM particles are t
 heorized to interact and produce standard model particles\, like gamma ray
 s. So far\, no definitive gamma-ray signal has been detected\, but current
  experiments have started excluding several thermal WIMP models. I will di
 scuss the current status of DM searches with gamma-ray observatories like 
 the Fermi LAT and HAWC. I will also discuss how both future analysis with 
 current observatories and future observatories like CTA and SWGO will prob
 e thermal WIMP models for masses from 5 GeV to ~100 TeV.\n\nhttps://indico
 .icrr.u-tokyo.ac.jp/event/259/contributions/1523/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1523/
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