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Radon Removal in XENONnT down to the Solar Neutrino Level

Title: Radon Removal in XENONnT down to the Solar Neutrino Level
Authors: Aprile, E. (Elena); Aalbers, J. (Jelle); Abe, K.; Maouloud, S.A.; Althüser, L. (Lutz); Andrieu, B. (Bernard); Angelino, E. (Emanuele); Martin, D.A. (David); Arneodo, F. (Francesco); Baudis, L. (Laura); Bazyk, M. (Marina); Bellagamba, L.; Biondi, R. (Riccardo); Bismark, A. (Alexander); Böse, K. (Kai); Softley-Brown , A. (Adam); Bruno, G. (Gianmarco); Budnik, R. (Ran); Cai, C.; Capelli, C. (Chiara); Cardoso, J.M.R. (João); Cimental Chávez, A.P. (Andrea); Colijn, A. (Auke); Conrad, J. (Jan); Cuenca Garcia, J.J. (Jose); D'Andrea, V. (Valerio); García, L.D. (Layos); Decowski, M.P. (Michal); Deisting, A. (Alexander); Donato, C.D. (Chiara); Gangi, P.D. (Pietro); Diglio, S. (Sara); Eitel, K. (Klaus); Morabit, S.E. (Saad); Elykov, A. (Alexey); Ferella, A.D. (Alfredo); Ferrari, C. (Cecilia); Fischer, H. (Horst); Flehmke, T. (Torben); Flierman, M. (Maricke); Fulgione, W. (Walter); Fuselli, C. (Carlo); Gaemers, P. (Peter); Gaior, R. (Romain); Galloway, M. (Michelle); Gao, F. (Fei); Ghosh, S. (Sayan); Giacomobono, R. (Roberto); Glade-Beucke, R. (Robin); Grandi, L. (Luca); Grigat, J. (Jaron); Guan, H. (Husheng); Guida, M. (Matteo); Gyorgy, P. (Peter); Hammann, R. (Robert); Higuera, A. (Aaron); Hils, C. (Christopher); Hötzsch, L. (Luisa); Hood, N. (Noah); Iacovacci, M. (Michele); Itow, Y. (Yoshitaka); Jakob, J. (Johanna); Jörg, F. (Florian); Kaminaga, Y. (Yoshino); Kara, M. (Melih); Kavrigin, P. (Pavel); Kazama, S. (Shingo); Kharbanda, P. (Pranati); Kobayashi, M. (Masatoshi); Koke, D. (David); Kopec, A. (Abigail); Landsman, H. (Hagar); Lang, R.F. (Rafael); Levinson, L. (Lorne); Li, I. (Ivy); Li, S. (Shengchao); Liang, S. (Shixiao); Liang, Z. (Zhenhao); Lin, Y. (Ying-Ting); Lindemann, S. (Sebastian); Lindner, M. (Manfred); Liu, K. (Kexin); Liu, M.; Loizeau, J. (Johan); Lombardi, F. (Francesco); Long, J. (Jianyu); Lopes, J.A.M.; Luce, T. (Tiffany); Ma, Y. (Yue); Macolino, C. (Carla); Mahlstedt, J. (Joern); Mancuso, A. (Andrea); Manenti, L. (Laura); Marignetti, F. (Fabrizio); Marrodán Undagoitia, T. (Teresa); Martens, K. (Kai); Masbou, J. (Julien); Masson, E. (Erwann); Mastroianni, S. (Stefano); Melchiorre, A. (Andrea); Merz, J. (Johannes); Messina, M. (Marcello); Michael, A.; Miuchi, K. (Kentaro); Molinario, A. (Andrea); Moriyama, S. (Shigetaka); Dundas Morå, K. (Knut); Mosbacher, Y.; Murra, M. (Michael); Müller, J. (Julia); Ni, K. (Kaixuan); Oberlack, U. (Uwe); Paetsch, B. (Barbara); Pan, Y. (Yongyu); Pellegrini, Q. (Quentin); Mota Peres, R.J. (Ricardo); Peters, C.; Pienaar, J. (Jacques); Pierre, M. (Maxime); Plante, G. (Guillaume); Pollmann, T.R. (Tina); Principe, L. (Lorenzo); Qi, J. (Jianyang); Qin, J. (Juehang); Ramírez García, D. (Diego); Rajado Silva, M. (Mariana); Singh, R. (Riya); Sanchez, L. (Luis); Santos, J.M.F.D.; Sarnoff, I. (Isaac); Sartorelli, G. (Gabriella); Schreiner, J.; Schulte, D.; Schulte, P. (Philipp); Schulze Eißing, H. (Henning); Schumann, M. (Marc); Scotto Lavina, L. (Luca); Selvi, M. (Marco); Semeria, F. (Franco); Chaguine, P. (Petr); Shi, S. (Shenyang); Shi, J.; Silva, M. (Miguel); Simgen, H. (Hardy); Szyszka, C.; Takeda, A. (Atsushi); Takeuchi, Y. (Yasuo); Tan, P.L. (Pueh); Thers, D. (Dominique); Toschi, F. (Francesco); Trinchero, G.C. (Gian); Tunnell, C. (Christopher); Tönnies, F. (Florian); Valerius, K. (Kathrin); Vecchi, S. (Stefania); Vetter, S. (Sebastian); Villazon Solar, F.; Volta, G. (Giovanni); Weinheimer, C. (Christian); Weiss, M. (Micha); Wenz, D. (Daniel); Wittweg, C. (Christian); Wu, V.H.S.; Xing, Y. (Yajing); Xu, D. (Dacheng); Xu, Z. (Zihao); Yamashita, M. (Masaki); Yang, L. (Liang); Ye, J. (Jingqiang); Yuan, L. (Lanqing); Zavattini, G. (Guido); Zhong, M. (Min)
Contributors: Universitäts- und Landesbibliothek Münster
Publication Year: 2026
Collection: Münster University (WWU): miami
Subject Terms: Alpha decay; Dark matter; Dark matter direct detection; Particle dark matter; Particle interactions; Phase separation; Solar neutrinos; Cryogenics; Multi-purpose particle detectors; Neutrino detection; Particle decays; Scintillators; ddc:530; info:eu-repo/classification/ddc/530; Physics
Description: The XENONnT experiment has achieved an exceptionally low 222Rn activity concentration within its inner 5.9 tonne liquid xenon detector of (0.90±0.02 stat±0.07 syst) μ⁢Bq kg−1, equivalent to about 430 222Rn atoms per tonne of xenon. This was achieved by active online radon removal via cryogenic distillation after stringent material selection. The achieved 222Rn activity concentration is 5 times lower than that in other currently operational multitonne liquid xenon detectors engaged in dark matter searches. This breakthrough enables the pursuit of various rare event searches that lie beyond the confines of the standard model of particle physics, with world-leading sensitivity. The ultralow 222Rn levels have diminished the radon-induced background rate in the detector to a point where it is for the first time comparable to the solar neutrino-induced background, which is poised to become the primary irreducible background in liquid xenon-based detectors.
Document Type: article in journal/newspaper
File Description: application/pdf
Language: English
DOI: 10.17879/70968424346
Availability: https://nbn-resolving.org/urn:nbn:de:hbz:6-70958481788; https://doi.org/10.17879/70968424346; https://miami.uni-muenster.de/Record/0a552485-3ab4-4bd0-b2ce-91343bb99d62; https://repositorium.uni-muenster.de/transfer/miami/0a552485-3ab4-4bd0-b2ce-91343bb99d62
Rights: CC BY 4.0 ; info:eu-repo/semantics/openAccess
Accession Number: edsbas.79BBC435
Database: BASE