XENON Collaboration,E. Aprile,J. Aalbers,K. Abe,S. Ahmed Maouloud,L. Althueser,B. Andrieu,E. Angelino,J. R. Angevaare,V. C. Antochi,D. Antón Martin,F. Arneodo,M. Balata,L. Baudis,A. L. Baxter,M. Bazyk,L. Bellagamba,R. Biondi,A. Bismark,E. J. Brookes,A. Brown,S. Bruenner,G. Bruno,R. Budnik,T. K. Bui,C. Cai,J. M. R. Cardoso,F. Cassese,A. Chiarini,D. Cichon,A. P. Cimental Chavez,A. P. Colijn,J. Conrad,R. Corrieri,J. J. Cuenca-García,J. P. Cussonneau,O. Dadoun,V. D'Andrea,M. P. Decowski,B. De Fazio,P. Di Gangi,S. Diglio,J. M. Disdier,D. Douillet,K. Eitel,A. Elykov,S. Farrell,A. D. Ferella,C. Ferrari,H. Fischer,M. Flierman,S. Form,D. Front,W. Fulgione,C. Fuselli,P. Gaemers,R. Gaior,A. Gallo Rosso,M. Galloway,F. Gao,R. Gardner,N. Garroum,R. Glade-Beucke,L. Grandi,J. Grigat,H. Guan,M. Guerzoni,M. Guida,R. Hammann,A. Higuera,C. Hils,L. Hoetzsch,N. F. Hood,J. Howlett,C. Huhmann,M. Iacovacci,G. Iaquaniello,L. Iven,Y. Itow,J. Jakob,F. Joerg,A. Joy,M. Kara,P. Kavrigin,S. Kazama,M. Kobayashi,G. Koltman,A. Kopec,F. Kuger,H. Landsman,R. F. Lang,L. Levinson,I. Li,S. Li,S. Liang,S. Lindemann,M. Lindner,K. Liu,J. Loizeau,F. Lombardi,J. Long,J. A. M. Lopes,Y. Ma,C. Macolino,J. Mahlstedt,A. Mancuso,L. Manenti,F. Marignetti,T. Marrodán Undagoitia,P. Martella,K. Martens,J. Masbou,D. Masson,E. Masson,S. Mastroianni,E. Mele,M. Messina,R. Michinelli,K. Miuchi,A. Molinario,S. Moriyama,K. Morå,Y. Mosbacher,M. Murra,J. Müller,K. Ni,S. Nisi,U. Oberlack,D. Orlandi,R. Othegraven,B. Paetsch,J. Palacio,S. Parlati,P. Paschos,Q. Pellegrini,R. Peres,C. Peters,J. Pienaar,M. Pierre,G. Plante,T. R. Pollmann,J. Qi,J. Qin,D. Ramírez García,M. Rynge,J. Shi,R. Singh,L. Sanchez,J. M. F. dos Santos,I. Sarnoff,G. Sartorelli,J. Schreiner,D. Schulte,P. Schulte,H. Schulze Eißing,M. Schumann,L. Scotto Lavina,M. Selvi,F. Semeria,P. Shagin,S. Shi,E. Shockley,M. Silva,H. Simgen,J. Stephen,M. Stern,B. K. Stillwell,A. Takeda,P. -L. Tan,D. Tatananni,A. Terliuk,D. Thers,F. Toschi,G. Trinchero,C. Tunnell,F. Tönnies,K. Valerius,G. Volta,C. Weinheimer,M. Weiss,D. Wenz,J. Westermann,C. Wittweg,T. Wolf,V. H. S. Wu,Y. Xing,D. Xu,Z. Xu,M. Yamashita,L. Yang,J. Ye,L. Yuan,G. Zavattini,M. Zhong,T. Zhu
Bulletin of the American Physical Society(2024)
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Abstract
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 5.9 tonnes of cryogenic liquid xenon (8.5
tonnes 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.
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