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    UCLA Dark Matter 2020 Conference

    Mar 25 – 28, 2020
    UCLA
    US/Pacific timezone

    dm20@physics.ucla.edu

    Session

    Session 4

    4
    Mar 25, 2020, 4:30 PM
    PAB- 1-425 (UCLA)

    PAB- 1-425

    UCLA

    UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095

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    1. 108. Dark Matter Detection with Liquid Xenon
      Prof. Elena Aprile (Columbia U.)
      3/25/20, 4:30 PM
      Non-directional direct dark matter detection
      Talk

      Detection of a Dark Matter signal in an ultra-low background terrestrial detector will provide the most direct evidence of its existence and will represent a ground-breaking discovery in physics and cosmology. Among the variety of dark matter detectors, liquid xenon time projection chambers have shown to be the most sensitive, thanks to a combination of very large target mass, ultra-low...

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    2. 110. Direct Detection with Argon
      Cristiano Galbiati (Princeton University)
      3/25/20, 5:00 PM
      Talk

      Overview of direct dark matter experiments using argon as target.

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    3. 111. Direct detection without noble gases
      Bernard Sadoulet (University of California, Berkeley)
      3/25/20, 5:30 PM
      Talk
    4. 112. New ideas for Sub-GeV dark matter direct detection
      Rouven Essig
      3/25/20, 6:00 PM
      Talk
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