A next-generation liquid xenon observatory for dark matter and neutrino physics
- NázevTitle
- A next-generation liquid xenon observatory for dark matter and neutrino physicsA next-generation liquid xenon observatory for dark matter and neutrino physics
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- J. Aalbers, S. S. AbdusSalam, K. Abe, X. Aerne, F. Šimkovic
- Klíčová slovaKeywords
- double beta decay, semi-leptonic weak, dual-phase xenon, half-life values, annual modulation, ionization yield, solar neutrinos, electromagnetic-interactions, cryogenic distillation, chromatographic system
- DOIDOI
- 10.1088/1361-6471/ac841a
- Časopis / citaceJournal / citation
- Journal of Physics G: Nuclear and Particle Physics 50(1), 013001 (2023) · ISSN 0954-3899
- RokYear
- 2023
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
- CitovánoCited by
- 223 (INSPIRE-HEP)
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
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.
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.