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

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doi:10.1088/1361-6471/ac841a

Title: A next-generation liquid xenon observatory for dark matter and neutrino physics

Journal Article · Thu Dec 22 00:00:00 EST 2022 · Journal of Physics. G, Nuclear and Particle Physics

DOI:https://doi.org/10.1088/1361-6471/ac841a· OSTI ID:1854776

Aalbers, J. ^[1]; AbdusSalam, S. S.; Abe, K.; Aerne, V.; Agostini, F.; Ahmed Maouloud, S.; Akerib, D. S.; Akimov, D. Y.; Akshat, J.; Al Musalhi, A. K.; Alder, F.; Alsum, S. K.; Althueser, L.; Amarasinghe, C. S.; Amaro, F. D.; Ames, A.; Anderson, T. J.; Andrieu, B.; Angelides, N.; Angelino, E. more »

SLAC National Accelerator Laboratory, Menlo Park, CA (United States); Stanford University, CA (United States); XLZD Collaboration. et al.

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.

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Research Organization:: Brookhaven National Laboratory (BNL), Upton, NY (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Contributing Organization:: XLZD Collaboration

Grant/Contract Number:: AC02-05CH11231; AC02-07CH11359; AC02-76SF00515; AC52-07NA27344; FG02-00ER41132; FG02-10ER46709; NA0003180; SC0006605; SC0008475; SC0009999; SC0010010; SC0010072; SC0010813; SC0011640; SC0011702; SC0012161; SC0012447; SC0012704; SC0013542; SC0014223; SC0015535; SC0015708; SC0018982; SC0019066; SC0020216; UW PRJ82AJ; SC0019193

OSTI ID:: 1854776

Alternate ID(s):: OSTI ID: 1902931; OSTI ID: 1995075

Report Number(s):: INT-PUB-22-003; FERMILAB-PUB-22-112-PPD-QIS-T; arXiv:2203.02309; oai:inspirehep.net:2046565; TRN: US2304959

Journal Information:: Journal of Physics. G, Nuclear and Particle Physics, Vol. 50, Issue 1; ISSN 0954-3899

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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