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18–24 Jun 2017
UC Irvine, Irvine, CA, USA
US/Pacific timezone

DARWIN: a 50-Ton Liquid Xenon Detector for Dark Matter and Neutrino Physics

23 Jun 2017, 10:45
15m
Pacific Ballroom C (UC Irvine, Irvine, CA, USA)

Pacific Ballroom C

UC Irvine, Irvine, CA, USA

Working Group Sessions Neutrino Physics Working Group Working Group: Neutrino Physics

Speaker

Prof. Kaixuan Ni (UC San Diego)

Description

DARWIN is the next generation liquid xenon experiment to probe the weak interactions for dark matter and neutrino physics. With a target mass ten times more than the current world’s largest liquid xenon detector (XENON1T), DARWIN will probe the WIMP-nucleon cross section down to the 10^-49 cm^2 region, measure the solar pp-neutrino flux down to sub-percent precision, probe the neutrino-nucleus coherent scattering, and search for neutrinoless double beta decays from more than 3.5-ton of Xe-136. The experiment is currently in the design phase. The technical challenges, possible solutions and design details will be presented.

Primary author

Prof. Kaixuan Ni (UC San Diego)

Presentation materials