Search for New Physics in Electronic Recoil Data from XENONnT.

E. Aprile, K. Abe,F. Agostini,S. Ahmed Maouloud, L. Althueser, B. Andrieu, E. Angelino,J. R. Angevaare,V. C. Antochi,D. Antón Martin,F. Arneodo,L. Baudis, A. L. Baxter,L. Bellagamba,R. Biondi,A. Bismark,A. Brown, S. Bruenner, G. Bruno,R. Budnik,T. K. Bui, C. Cai,C. Capelli,J. M. R. Cardoso,D. Cichon,M. Clark,A. P. Colijn,J. Conrad, J. J. Cuenca-García,J. P. Cussonneau,V. D'Andrea,M. P. Decowski,P. Di Gangi,S. Di Pede,A. Di Giovanni,R. Di Stefano, S. Diglio,K. Eitel,A. Elykov,S. Farrell,A. D. Ferella,C. Ferrari,H. Fischer, W. Fulgione, P. Gaemers,R. Gaior,A. Gallo Rosso,M. Galloway,F. Gao, R. Gardner, R. Glade-Beucke, L. Grandi, J. Grigat,M. Guida,R. Hammann,A. Higuera, C. Hils, L. Hoetzsch,J. Howlett,M. Iacovacci, Y. Itow,J. Jakob,F. Joerg,A. Joy,N. Kato,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,K. Martens,J. Masbou,D. Masson, E. Masson,S. Mastroianni,M. Messina, K. Miuchi, K. Mizukoshi, A. Molinario,S. Moriyama,K. Morå, Y. Mosbacher, M. Murra, J. Müller,K. Ni,U. Oberlack, B. Paetsch,J. Palacio, P. Paschos,R. Peres, C. Peters,J. Pienaar,M. Pierre, V. Pizzella, G. Plante,J. Qi,J. Qin,D. Ramírez García, S. Reichard, A. Rocchetti,N. Rupp,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, A. Takeda,P. -L. Tan, A. Terliuk,D. Thers,F. Toschi, G. Trinchero,C. Tunnell, F. Tönnies, K. Valerius,G. Volta,Y. Wei, C. Weinheimer,M. Weiss, D. Wenz,C. Wittweg,T. Wolf,D. Xu,Z. Xu,M. Yamashita,L. Yang,J. Ye, L. Yuan, G. Zavattini,M. Zhong,T. Zhu

Physical review letters(2022)

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摘要
We report on a blinded analysis of low-energy electronic recoil data from the first science run of the XENONnT dark matter experiment. Novel subsystems and the increased 5.9 ton liquid xenon target reduced the background in the (1, 30) keV search region to (15.8±1.3)  events/(ton×year×keV), the lowest ever achieved in a dark matter detector and ∼5 times lower than in XENON1T. With an exposure of 1.16 ton-years, we observe no excess above background and set stringent new limits on solar axions, an enhanced neutrino magnetic moment, and bosonic dark matter.
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electronic recoil data,xenonnt,new physics
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