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25–28 Mar 2020
UCLA
US/Pacific timezone

Physics reach of the LUX-Zeplin Dark Matter Experiment

27 Mar 2020, 17:15
15m
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 15

Speaker

Maria Elena Monzani (SLAC)

Description

The nature and origin of Dark Matter are among the most compelling mysteries of contemporary science. For over three decades, physicists have been trying to detect Dark Matter particles via collisions on target nuclei, with little success.
The LZ collaboration is building a massive Dark Matter detector, which is currently being installed at the 4850 level of the Sanford Underground Research Facility in Lead, South Dakota. This detector features 7 active tons of target nuclei and uses the established liquid xenon TPC technology to achieve unprecedented sensitivity to a wide range of Dark Matter candidates. In this talk I will review the physics reach of the LZ experiment.

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