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SUMMARY:La Trobada: Astrophysical probes for Dark Matter searches
DTSTART;VALUE=DATE-TIME:20131129T094500Z
DTEND;VALUE=DATE-TIME:20131129T111500Z
DTSTAMP;VALUE=DATE-TIME:20261023T131831Z
UID:indico-event-2030@indico.ific.uv.es
DESCRIPTION:\n    Current LCDM cosmological paradigm describes most of the
  Universe's matter content as made of an unknown\, non-electromagnetically
  interacting\, non-baryonic (*dark*) component. The nature of the Dark Mat
 ter particle is studied through a host of diverse technique\, including di
 rect production at LHC\, underground recoil experiments (direct detection)
 \, and indirect probes\, typically of astrophysical nature. After a brief 
 introduction\, in this talk I will describe two astrophysical observables 
 which can be used to obtain information on different properties of the Dar
 k Matter (DM): i) Combining microlensing observations of the galactic bulg
 e with rotation curves of the Milky Way\, it is possible to constrain the 
 local DM density and more mildly the DM profile of our galaxy's halo\, com
 plementing the results obtained with other techniques. ii) Cosmic Microwav
 e Background (CMB) observations can bring information about the self-annih
 ilation properties of DM particles\, complementing indirect searches typic
 ally pursued through gamma ray or charged particles in local targets.\n\nh
 ttps://indico.ific.uv.es/event/2030/
LOCATION:IFIC Seminar Room 1.1.1
URL:https://indico.ific.uv.es/event/2030/
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