The XENONnT Dark Matter Experiment

التفاصيل البيبلوغرافية
العنوان: The XENONnT Dark Matter Experiment
المؤلفون: Aprile, E, Aalbers, J, Abe, K, Ahmed Maouloud, S, Althueser, L, Andrieu, B, Angelino, E, Angevaare, J.R, Antochi, V.C, Martin, D. Antón, Arneodo, F, Balata, M, Baudis, L, Baxter, A.L, Bazyk, M, Bellagamba, L, Biondi, R, Bismark, A, Brookes, E.J, Brown, A, Bruenner, S, Bruno, G, Budnik, R, Bui, T.K, Cai, C, Cardoso, J.M.R, Cassese, F, Chiarini, A, Cichon, D, Chavez, A.P. Cimental, Colijn, A.P, Conrad, J, Corrieri, R, Cuenca-García, J.J, Cussonneau, J.P, Dadoun, O, d'Andrea, V, Decowski, M.P, de Fazio, B, Di Gangi, P, Diglio, S, Disdier, J.M, Douillet, D, Eitel, K, Elykov, A, Farrell, S, Ferella, A.D, Ferrari, C, Fischer, H, Flierman, M, Form, S, Front, D, Fulgione, W, Fuselli, C, Gaemers, P, Gaior, R, Gallo Rosso, A, 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, N.F, 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, R.F, Levinson, L, Li, I, Li, S, Liang, S, Lindemann, S, Lindner, M, Liu, K, Loizeau, J, Lombardi, F, Long, J, Lopes, J.A.M, Ma, Y, Macolino, C, Mahlstedt, J, Mancuso, A, Manenti, L, Marignetti, F, Marrodán Undagoitia, T, Martella, P, Martens, K, Masbou, J, Masson, D, Masson, E, Mastroianni, S, Mele, E, Messina, M, Michinelli, R, Miuchi, K, Molinario, A, Moriyama, S, Morå, K, Mosbacher, Y, Murra, M, Müller, J, Ni, K, Nisi, S, Oberlack, U, Orlandi, D, Othegraven, R, Paetsch, B, Palacio, J, Parlati, S, Paschos, P, Pellegrini, Q, Peres, R, Peters, C, Pienaar, J, Pierre, M, Plante, G, Pollmann, T.R, Qi, J, Qin, J, Ramírez García, D, Rynge, M, Shi, J, Singh, R, Sanchez, L, dos Santos, J.M.F, Sarnoff, I, Sartorelli, G, Schreiner, J, Schulte, D, Schulte, P, Eißing, H. Schulze, Schumann, M, Scotto Lavina, L, Selvi, M, Semeria, F, Shagin, P, Shi, S, Shockley, E, Silva, M, Simgen, H, Stephen, J, Stern, M, Stillwell, B.K, Takeda, A, Tan, P.-L, Tatananni, D, Terliuk, A, Thers, D, Toschi, F, Trinchero, G, Tunnell, C, Tönnies, F, Valerius, K, Volta, G, Weinheimer, C, Weiss, M, Wenz, D, Westermann, J, Wittweg, C, Wolf, T, Wu, V.H.S, Xing, Y, Xu, D, Xu, Z, Yamashita, M, Yang, L, Ye, J, Yuan, L, Zavattini, G, Zhong, M, Zhu, T
المساهمون: Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom Paris (IMT)-Institut Mines-Télécom Paris (IMT)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), XENON
المصدر: https://hal.science/hal-04479882Test ; 2024.
بيانات النشر: HAL CCSD
سنة النشر: 2024
مصطلحات موضوعية: xenon, liquid, detector, performance, WIMP, dark matter, time projection chamber, sensitivity, cryogenics, upgrade, radon, Gran Sasso, background, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
الوصف: International audience ; 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.
نوع الوثيقة: report
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2402.10446; hal-04479882; https://hal.science/hal-04479882Test; ARXIV: 2402.10446; INSPIRE: 2759141
الإتاحة: https://hal.science/hal-04479882Test
رقم الانضمام: edsbas.48BB9DBF
قاعدة البيانات: BASE