| Title: |
The XENONnT dark matter experiment |
| Authors: |
Aprile, E; Aalbers, J; Abe, K; Ahmed Maouloud, S; Althueser, L; Andrieu, B; Angelino, E; Angevaare, JR; Antochi, VC; Antón Martin, D; Arneodo, F; Balata, M; Baudis, L; Baxter, AL; Bazyk, M; Bellagamba, L; Biondi, R; Bismark, A; Brookes, EJ; Brown, A; Bruenner, S; Bruno, G; Budnik, R; Bui, TK; Cai, C; Cardoso, JMR; Cassese, F; Chiarini, A; Cichon, D; Cimental Chavez, AP; Colijn, AP; Conrad, J; Corrieri, R; Cuenca-García, JJ; Cussonneau, JP; Dadoun, O; D’Andrea, V; Decowski, MP; De Fazio, B; Gangi, P Di; Diglio, S; Disdier, JM; Douillet, D; Eitel, K; Elykov, A; Farrell, S; Ferella, AD; Ferrari, C; Fischer, H; Flierman, M; Form, S; Front, D; Fulgione, W; Fuselli, C; Gaemers, P; Gaior, R; Rosso, A Gallo; Galloway, M; Gao, F; Gardner, R; Garroum, N; Glade-Beucke, R; Grandi, L; Grigat, J; Guan, H; Guerzoni, M; Guida, M; Hammann, R; Higuera, A; Hils, C; Hoetzsch, L; Hood, NF; Howlett, J; Huhmann, C; Iacovacci, M; Iaquaniello, G; Iven, L; Itow, Y; Jakob, J; Joerg, F; Joy, A; Kara, M; Kavrigin, P; Kazama, S; Kobayashi, M; Koltman, G; Kopec, A; Kuger, F; Landsman, H; Lang, RF; Levinson, L; Li, I; Li, S; Liang, S; Lindemann, S; Lindner, M; Liu, K; Loizeau, J; Lombardi, F; Long, J |
| Source: |
European Physical Journal C, vol 84, iss 8 |
| Publisher Information: |
eScholarship, University of California |
| Publication Year: |
2024 |
| Collection: |
University of California: eScholarship |
| Subject Terms: |
5106 Nuclear and Plasma Physics (for-2020); 5107 Particle and High Energy Physics (for-2020); 51 Physical Sciences (for-2020); XENON Collaboration; 0202 Atomic; Molecular; Nuclear; Particle and Plasma Physics (for); 0206 Quantum Physics (for); Nuclear & Particles Physics (science-metrix); 5101 Astronomical sciences (for-2020); 5102 Atomic; molecular and optical physics (for-2020) |
| Description: |
The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, planned to be an upgrade of its predecessor XENON1T. It features an active target of 5.9tonnes of cryogenic liquid xenon (8.5tonnes total mass in cryostat). The experiment is expected to extend the sensitivity to WIMP dark matter by more than an order of magnitude compared to XENON1T, thanks to the larger active mass and the significantly reduced background, improved by novel systems such as a radon removal plant and a neutron veto. This article describes the XENONnT experiment and its sub-systems in detail and reports on the detector performance during the first science run. |
| Document Type: |
article in journal/newspaper |
| File Description: |
application/pdf |
| Language: |
unknown |
| Relation: |
qt8qq7642j; https://escholarship.org/uc/item/8qq7642j; https://escholarship.org/content/qt8qq7642j/qt8qq7642j.pdf |
| DOI: |
10.1140/epjc/s10052-024-12982-5 |
| Availability: |
https://escholarship.org/uc/item/8qq7642j; https://escholarship.org/content/qt8qq7642j/qt8qq7642j.pdf; https://doi.org/10.1140/epjc/s10052-024-12982-5 |
| Rights: |
CC-BY |
| Accession Number: |
edsbas.5B8B7940 |
| Database: |
BASE |