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

0572223 - FZÚ 2024 RIV US eng J - Článek v odborném periodiku
Aalbers, J. - AbdusSalam, S.S. - Abe, K. - Pěč, Viktor … celkem 599 autorů
A next-generation liquid xenon observatory for dark matter and neutrino physics.
Journal of Physics G-Nuclear and Particle Physics. Roč. 50, č. 1 (2023), č. článku 013001. ISSN 0954-3899. E-ISSN 1361-6471
Institucionální podpora: RVO:68378271
Klíčová slova: dark matter * neutrinoless double-beta decay * neutrinos * supernova * direct detection * astroparticle physics * xenon
Obor OECD: Particles and field physics
Impakt faktor: 3.5, rok: 2022
Způsob publikování: Open access

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.
Trvalý link: https://hdl.handle.net/11104/0350303