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SUMMARY:Particle and halo model uncertainties in direct dark matter detect
 ion
DTSTART;VALUE=DATE-TIME:20191111T064500Z
DTEND;VALUE=DATE-TIME:20191111T071500Z
DTSTAMP;VALUE=DATE-TIME:20250110T182859Z
UID:indico-contribution-1659@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Graciela Gelmini (UCLA)\nAfter briefly reviewing the
  WIMP status as dark matter (DM) candidate\, I will mention how the impact
   of the neutrino floor on the direct detection (DD) reach depends on the 
 type of WIMP-nucleus interaction and mass\, and then how  a DD signal woul
 d translate into properties of the DM local velocity distribution\, allowi
 ng to compare different DD data sets  through these predictions (in  a “
 halo-independent” analysis complementary to the usual halo-dependent met
 hod).\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1659/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1659/
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