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A next-generation liquid xenon observatory for dark matter and neutrino physics
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0003-1331-2890
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC). Princeton University, United States of America.ORCID iD: 0000-0001-8971-834x
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0001-9984-4411
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).ORCID iD: 0000-0002-4251-2229
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Number of Authors: 5992023 (English)In: Journal of Physics G: Nuclear and Particle Physics, ISSN 0954-3899, E-ISSN 1361-6471, Vol. 50, no 1, article id 013001Article, review/survey (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2023. Vol. 50, no 1, article id 013001
Keywords [en]
dark matter, neutrinoless double-beta decay, neutrinos, supernova, direct detection, astroparticle physics, xenon
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-215894DOI: 10.1088/1361-6471/ac841aISI: 000928191300001Scopus ID: 2-s2.0-85145605367OAI: oai:DiVA.org:su-215894DiVA, id: diva2:1746802
Available from: 2023-03-29 Created: 2023-03-29 Last updated: 2023-03-29Bibliographically approved

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Antochi, Vasile C.Blanco, CarlosConrad, JanEmken, TimonJoy, AshleyMahlstedt, JörnSmirnov, JuriTan, Pueh-Leng

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Antochi, Vasile C.Blanco, CarlosConrad, JanEmken, TimonJoy, AshleyMahlstedt, JörnSmirnov, JuriTan, Pueh-Leng
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Department of PhysicsThe Oskar Klein Centre for Cosmo Particle Physics (OKC)
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Journal of Physics G: Nuclear and Particle Physics
Astronomy, Astrophysics and Cosmology

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