14th International Conference on Topics in Astroparticle and Underground Physics | |
The LZ dark matter experiment | |
物理学;天文学 | |
McKinsey, D.N.^1 | |
Department of Physics, 441 LeConte Hall, University of California, Berkeley | |
CA | |
94720, United States^1 | |
关键词: Dark matter; Dark matter detectors; Direct detection; Fusion process; Neutrinoless double-beta decays; Solar neutrino; Two phase; | |
Others : https://iopscience.iop.org/article/10.1088/1742-6596/718/4/042039/pdf DOI : 10.1088/1742-6596/718/4/042039 |
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学科分类:天文学(综合) | |
来源: IOP | |
【 摘 要 】
The LUX and ZEPLIN collaborations have merged to construct a 7 tonne two-phase Xe dark matter detector, known as LUX-ZEPLIN or LZ. Chosen as one of the Generation 2 suite of dark matter direct detection experiments, LZ will probe spin-independent WIMP-nucleon cross sections down to 2 ×10-48cm2at 50 GeV/c2within 3 years of operation, covering a substantial range of theoretically-motivated dark matter candidates. Along with dark matter interactions with Xe nuclei, LZ will also be sensitive to solar neutrinos emitted by the pp fusion process in the sun, neutrinos emitted by a nearby supernova and detected by coherent neutrino-nucleus scattering, certain classes of axions and axion-like particles, and neutrinoless double-beta decay of136Xe. The design of LZ is presented, along with its expected backgrounds and projected sensitivity.
【 预 览 】
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