First Search for Light Dark Matter in the Neutrino Fog with XENONnT

We search for dark matter (DM) with a mass [3,12] GeV/c^{2} using an exposure of 3.51 tonne year with the XENONnT experiment. We consider spin-independent DM-nucleon interactions mediated by a heavy or light mediator, spin-dependent DM-neutron interactions, momentum-dependent DM scattering, and mirror DM. Using a lowered energy threshold compared to the previous weakly interacting massive particle search, a blind analysis of [0.5, 5.0] keV nuclear recoil events reveals no significant signal excess over the background. XENONnT excludes spin-independent DM-nucleon cross sections >2.5×10^{-45} cm^{2} at 90% confidence level for 6 GeV/c^{2} DM. In the considered mass range, the DM sensitivity approaches the "neutrino fog," the limitation where neutrinos produce a signal that is indistinguishable from that of light DM-xenon nucleus scattering.

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Publication Details

Journal
Physical Review Letters
Published
2025-03-20
DOI
https://doi.org/10.1103/physrevlett.134.111802
Citations
14
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
26.18

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article

First Search for Light Dark Matter in the Neutrino Fog with XENONnT

U Oberlack, M Zhong, M. Kara, K. Miuchi et al.
14 citations
Physical Review Letters
Dark Matter and Cosmic Phenomena
26.18
article

First Search for Light Dark Matter in the Neutrino Fog with XENONnT

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

Abstract

We search for dark matter (DM) with a mass [3,12] GeV/c^{2} using an exposure of 3.51 tonne year with the XENONnT experiment. We consider spin-independent DM-nucleon interactions mediated by a heavy or light mediator, spin-dependent DM-neutron interactions, momentum-dependent DM scattering, and mirror DM. Using a lowered energy threshold compared to the previous weakly interacting massive particle search, a blind analysis of [0.5, 5.0] keV nuclear recoil events reveals no significant signal excess over the background. XENONnT excludes spin-independent DM-nucleon cross sections >2.5×10^{-45} cm^{2} at 90% confidence level for 6 GeV/c^{2} DM. In the considered mass range, the DM sensitivity approaches the "neutrino fog," the limitation where neutrinos produce a signal that is indistinguishable from that of light DM-xenon nucleus scattering.

Physical Review LettersVol. 134(11)
Karlsruhe Institute of Technology (DE), University of Fribourg (CH), Stockholm University (SE), University of Groningen (NL), Chinese University of Hong Kong (HK), 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), 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, 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, 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, Instituto Nacional de Ciência e Tecnologia: Física Nuclear e Aplicações, Conseil Régional des Pays de la Loire, Horizon 2020 Framework Programme, Japan Society for the Promotion of Science, 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
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Dark Matter and Cosmic Phenomena
26.18
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