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A next-generation liquid xenon observatory for dark matter and neutrino physics
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SYSNO ASEP 0572223 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title A next-generation liquid xenon observatory for dark matter and neutrino physics Author(s) Aalbers, J. (US)
AbdusSalam, S.S. (IR)
Abe, K. (JP)
Pěč, Viktor (FZU-D) ORCIDNumber of authors 599 Article number 013001 Source Title Journal of Physics G-Nuclear and Particle Physics. - : Institute of Physics Publishing - ISSN 0954-3899
Roč. 50, č. 1 (2023)Number of pages 116 s. Language eng - English Country US - United States Keywords dark matter ; neutrinoless double-beta decay ; neutrinos ; supernova ; direct detection ; astroparticle physics ; xenon Subject RIV BF - Elementary Particles and High Energy Physics OECD category Particles and field physics Method of publishing Open access Institutional support FZU-D - RVO:68378271 UT WOS 000928191300001 EID SCOPUS 85145605367 DOI 10.1088/1361-6471/ac841a Annotation The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for weakly interacting massive particles, while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector. Workplace Institute of Physics Contact Kristina Potocká, potocka@fzu.cz, Tel.: 220 318 579 Year of Publishing 2024 Electronic address https://hdl.handle.net/11104/0350303
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