Search for Light Dark Matter in Low-Energy Ionization Signals from XENONnT

We report on a blinded search for dark matter with single- and few-electron signals in the first science run of XENONnT relying on a novel detector response framework that is physics model dependent. We derive 90% confidence upper limits for dark matter-electron interactions. Heavy and light mediator cases are considered for the standard halo model and dark matter up-scattered in the Sun. We set stringent new limits on dark matter-electron scattering via a heavy mediator with a mass within 10-20 MeV/c^{2} and electron absorption of axionlike particles and dark photons for m_{χ} below 0.03 keV/c^{2}.

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Publication Details

Journal
Physical Review Letters
Published
2025-04-25
DOI
https://doi.org/10.1103/physrevlett.134.161004
Citations
15
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
28.05

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article

Search for Light Dark Matter in Low-Energy Ionization Signals from XENONnT

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15 citations
Physical Review Letters
Dark Matter and Cosmic Phenomena
28.05
article

Search for Light Dark Matter in Low-Energy Ionization Signals from XENONnT

M. Kara, K. Miuchi, F. Lombardi, G. Plante, K. Martens, V. H. S. Wu, C. Hils, L. J. Levinson, G. Trinchero, S. Moriyama, E. Aprile, Y. Itow, C. Wittweg, K. Eitel, F. Gao, R. Glade-Beucke, R. Budnik, J. Grigat, C. Szyszka, J. Qin, M. Yamashita, C. Capelli, Aya Takeda, E. Masson, F. Tönnies, Luisa Hötzsch, A. Molinario, J. J. Cuenca-García, M. Pierre, L. Althueser, C. Fuselli, L. Baudis, E. Angelino, K. Liu, Y. Mosbacher, S. Lindemann, R. Singh, A. Kopec, M. Flierman, P. Di Gangi, A. Bismark, A. Elykov, M. Galloway, W. Fulgione, J. Loizeau, A. D. Ferella, Y. Ma, F. Arneodo, D. Xu, M. Iacovacci, M. Guida, R Giacomobono, C. Peters, S. Li, M. P. Decowski, Jiaru Shi, Q. Pellegrini, L. Manenti, Y. Xing, A. Higuera, I. Sarnoff, S. Mastroianni, A. Deisting, C. Weinheimer, J. Masbou, S. Kazama, Fabrizio Marignetti, S. Ahmed Maouloud, D. Ramírez García, J. Aalbers, A. P. Colijn, J. M. R. Cardoso, M. Selvi, G. Bruno, S. Vecchi, R. F. Lang, K. Ni, D. Thers, V. D’Andrea, N. F. Hood, H. Simgen, M. Bazyk, Y Kaminaga, K. Boese, D. Wenz, J.M.F. dos Santos, G. Zavattini, T. Marrodán Undagoitia, R. Biondi, B. Paetsch, T. R. Pollmann, S. Liang, A. Brown, P. Schulte, P. Shagin, P. Kavrigin, M. Schümann, J. A. M. Lopes, D. Antón Martin, T.C. Luce, L. Bellagamba, Agnieszka Michael, M. Lindner, C. Tunnell, Jon F. Merz, C. Cai, P. Gaemers, K. Valerius, A. P. Cimental Chávez, U. Oberlack, L. Grandi, R. Peres, Florian Jörg, L Principe, S. el Morabit, M Rajado, T Flehmke, A Melchiorre, M. Messina, S. Shi, K. Abe, H. Fischer, Lina Yang, M. Silva, P.-L. Tan, Jan Conrad, A. Mancuso, F. Toschi, Jianyang Qi, C. Macolino, J. Pienaar, H. Landsman, D Koke, L. C. Daniel Garcia, R. Hammann, I. Li, H. Schulze Eißing, J. Jakob, S. Ghosh, M. Zhong, F. Semeria, J. Schreiner, J. Mahlstedt, G. Volta, G. Sartorelli, S. Diglio, J. Müller, M. Murra, K. Morå, R. Gaïor, H. Guan, L. Scotto Lavina, M. Weiss, F. I. Villazon Solar, L. Escudero Sanchez, Ye J, Ming Liu, C Di Donato, C. Ferrari, B. Andrieu, P Gyorgy, S Vetter, Z. Xu, M. Kobayashi, Y.-T. Lin, L. Yuan, J. Long, Y. Pan
article en
15 citations

Abstract

We report on a blinded search for dark matter with single- and few-electron signals in the first science run of XENONnT relying on a novel detector response framework that is physics model dependent. We derive 90% confidence upper limits for dark matter-electron interactions. Heavy and light mediator cases are considered for the standard halo model and dark matter up-scattered in the Sun. We set stringent new limits on dark matter-electron scattering via a heavy mediator with a mass within 10-20 MeV/c^{2} and electron absorption of axionlike particles and dark photons for m_{χ} below 0.03 keV/c^{2}.

Physical Review LettersVol. 134(16)
University of Fribourg (CH), Stockholm University (SE), University of Groningen (NL), Johannes Gutenberg University Mainz (DE), University of Ferrara (IT), University of Zurich (CH), Purdue University West Lafayette (US), University of Münster (DE), University of L'Aquila (IT), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso (IT), Westlake University (CN), University of California San Diego (US), Sorbonne Université (FR), University of Chicago (US), National Institute for Subatomic Physics (NL), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT), Chinese University of Hong Kong, Shenzhen (CN), AlbaNova (SE), Istituto Nazionale di Fisica Nucleare, Sezione di Bologna (IT), Gran Sasso Science Institute (IT), Max Planck Institute for Nuclear Physics (DE), Laboratoire Médiations (FR), Weizmann Institute of Science (IL), New York University (US), Nagoya University (JP), Kobe University (JP), Rice University (US), The University of Tokyo (JP), University of Coimbra (PT), Columbia University (US), University of Amsterdam (NL), University of Bologna (IT), Nantes Université (FR), Tsinghua University (CN)
National Science Foundation, Kavli Foundation, University of Chicago, Istituto Nazionale di Fisica Nucleare Sezione di Padova, San Diego Supercomputer Center, European Commission, Helmholtz-Gemeinschaft, Deutsche Forschungsgemeinschaft, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Weizmann Institute of Science, United States-Israel Binational Science Foundation, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Conseil Régional, Île-de-France, Knut och Alice Wallenbergs Stiftelse, Tsinghua University, Max-Planck-Gesellschaft, Centre National de la Recherche Scientifique, Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie, Istituto Nazionale di Fisica Nucleare, Horizon 2020 Framework Programme, Japan Society for the Promotion of Science, Fundação para a Ciência e a Tecnologia, Japan Science and Technology Agency, Instituto Nazionale di Fisica Nucleare, Institut National de Physique Nucléaire et de Physique des Particules, Laboratori Nazionali del Gran Sasso, H2020 Marie Skłodowska-Curie Actions
Openalex Percentile: Top 0%
Dark Matter and Cosmic Phenomena
28.05
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