25–28 Mar 2020
UCLA
US/Pacific timezone

Dark Matter Detection with Liquid Xenon

25 Mar 2020, 16:30
30m
PAB- 1-425 (UCLA)

PAB- 1-425

UCLA

UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095
Talk Non-directional direct dark matter detection Session 4

Speaker

Prof. Elena Aprile (Columbia U.)

Description

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 background and excellent signal-to-noise discrimination. Experiments based on this technology have led the field for the past decade. I will review the world leading results achieved with the first tonne scale experiment, XENON1T, before discussing sensitivity and discovery potential of the larger XENONnT and LZ expected to become operational this year.

Author

Prof. Elena Aprile (Columbia U.)

Presentation materials

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