DARWIN - a next-generation liquid xenon observatory for dark matter and neutrino physics

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作者
Thieme, Kevin [1 ]
机构
[1] Univ Zurich, Dept Phys, Winterthurerstr 190, Zurich, Switzerland
来源
37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021 | 2022年
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P1 [天文学];
学科分类号
0704 ;
摘要
Benefiting from more than a decade of experience in WIMP searches with dual-phase xenon time projection chambers, the DARWIN (DARk matter WImp search with liquid xenoN) collaboration intends to build a next-generation detector involving 50 tonnes (40 tonnes active) of xenon. The primary goal of the observatory is to explore the entire experimentally accessible parameter space for WIMP masses above 5 GeV/c(2) down to the irreducible neutrino floor. With its low energy threshold and ultra-low background level, DARWIN will be an excellent platform to search for various other rare interactions. These include the neutrinoless double beta decay of Xe-136, a high-precision measurement of the low-energy solar neutrino flux, as well as searches for solar axions and axion-like-particles. We present the detector concept, the sensitivity to the various science channels, and ongoing R&D efforts.
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