E Aprile, J Aalbers, K Abe, S Ahmed Maouloud, L Althueser, B Andrieu, E Angelino, D Antón Martin, F Arneodo, L Baudis, M Bazyk, L Bellagamba, R Biondi, A Bismark, K Boese, A Brown, G Bruno, R Budnik, C Cai, C Capelli, J M R Cardoso, A P Cimental Chávez, A P Colijn, J Conrad, J J Cuenca-García, V D'Andrea, L C Daniel Garcia, M P Decowski, A Deisting, C Di Donato, P Di Gangi, S Diglio, K Eitel, S El Morabit, A Elykov, A D Ferella, C Ferrari, H Fischer, T Flehmke, M Flierman, W Fulgione, C Fuselli, P Gaemers, R Gaior, M Galloway, F Gao, S Ghosh, R Giacomobono, R Glade-Beucke, L Grandi, J Grigat, H Guan, M Guida, P Gyorgy, R Hammann, A Higuera, C Hils, L Hoetzsch, N F Hood, M Iacovacci, Y Itow, J Jakob, F Joerg, Y Kaminaga, M Kara, P Kavrigin, S Kazama, M Kobayashi, D Koke, A Kopec, H Landsman, R F Lang, L Levinson, I Li, S Li, S Liang, Y-T Lin, S Lindemann, M Lindner, K Liu, M Liu, J Loizeau, F Lombardi, J Long, J A M Lopes, T Luce, Y Ma, C Macolino, J Mahlstedt, A Mancuso, L Manenti, F Marignetti, T Marrodán Undagoitia, K Martens, J Masbou, E Masson, S Mastroianni, A Melchiorre, J Merz, M Messina, A Michael, K Miuchi, A Molinario, S Moriyama, K Morå, Y Mosbacher, M Murra, J Müller, K Ni, U Oberlack, B Paetsch, Y Pan, Q Pellegrini, R Peres, C Peters, J Pienaar, M Pierre, G Plante, T R Pollmann, L Principe, J Qi, J Qin, D Ramírez García, M Rajado, R Singh, L Sanchez, J M F Dos Santos, I Sarnoff, G Sartorelli, J Schreiner, P Schulte, H Schulze Eißing, M Schumann, L Scotto Lavina, M Selvi, F Semeria, P Shagin, S Shi, J Shi, M Silva, H Simgen, C Szyszka, A Takeda, P-L Tan, D Thers, F Toschi, G Trinchero, C D Tunnell, F Tönnies, K Valerius, S Vecchi, S Vetter, F I Villazon Solar, G Volta, C Weinheimer, M Weiss, D Wenz, C Wittweg, V H S Wu, Y Xing, D Xu, Z Xu, M Yamashita, L Yang, J Ye, L Yuan, G Zavattini, M Zhong
{"title":"利用 XENONnT 首次在中微子迷雾中寻找轻暗物质。","authors":"E Aprile, J Aalbers, K Abe, S Ahmed Maouloud, L Althueser, B Andrieu, E Angelino, D Antón Martin, F Arneodo, L Baudis, M Bazyk, L Bellagamba, R Biondi, A Bismark, K Boese, A Brown, G Bruno, R Budnik, C Cai, C Capelli, J M R Cardoso, A P Cimental Chávez, A P Colijn, J Conrad, J J Cuenca-García, V D'Andrea, L C Daniel Garcia, M P Decowski, A Deisting, C Di Donato, P Di Gangi, S Diglio, K Eitel, S El Morabit, A Elykov, A D Ferella, C Ferrari, H Fischer, T Flehmke, M Flierman, W Fulgione, C Fuselli, P Gaemers, R Gaior, M Galloway, F Gao, S Ghosh, R Giacomobono, R Glade-Beucke, L Grandi, J Grigat, H Guan, M Guida, P Gyorgy, R Hammann, A Higuera, C Hils, L Hoetzsch, N F Hood, M Iacovacci, Y Itow, J Jakob, F Joerg, Y Kaminaga, M Kara, P Kavrigin, S Kazama, M Kobayashi, D Koke, A Kopec, H Landsman, R F Lang, L Levinson, I Li, S Li, S Liang, Y-T Lin, S Lindemann, M Lindner, K Liu, M Liu, J Loizeau, F Lombardi, J Long, J A M Lopes, T Luce, Y Ma, C Macolino, J Mahlstedt, A Mancuso, L Manenti, F Marignetti, T Marrodán Undagoitia, K Martens, J Masbou, E Masson, S Mastroianni, A Melchiorre, J Merz, M Messina, A Michael, K Miuchi, A Molinario, S Moriyama, K Morå, Y Mosbacher, M Murra, J Müller, K Ni, U Oberlack, B Paetsch, Y Pan, Q Pellegrini, R Peres, C Peters, J Pienaar, M Pierre, G Plante, T R Pollmann, L Principe, J Qi, J Qin, D Ramírez García, M Rajado, R Singh, L Sanchez, J M F Dos Santos, I Sarnoff, G Sartorelli, J Schreiner, P Schulte, H Schulze Eißing, M Schumann, L Scotto Lavina, M Selvi, F Semeria, P Shagin, S Shi, J Shi, M Silva, H Simgen, C Szyszka, A Takeda, P-L Tan, D Thers, F Toschi, G Trinchero, C D Tunnell, F Tönnies, K Valerius, S Vecchi, S Vetter, F I Villazon Solar, G Volta, C Weinheimer, M Weiss, D Wenz, C Wittweg, V H S Wu, Y Xing, D Xu, Z Xu, M Yamashita, L Yang, J Ye, L Yuan, G Zavattini, M Zhong","doi":"10.1103/PhysRevLett.134.111802","DOIUrl":null,"url":null,"abstract":"<p><p>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.</p>","PeriodicalId":20069,"journal":{"name":"Physical review letters","volume":"134 11","pages":"111802"},"PeriodicalIF":8.1000,"publicationDate":"2025-03-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"First Search for Light Dark Matter in the Neutrino Fog with XENONnT.\",\"authors\":\"E Aprile, J Aalbers, K Abe, S Ahmed Maouloud, L Althueser, B Andrieu, E Angelino, D Antón Martin, F Arneodo, L Baudis, M Bazyk, L Bellagamba, R Biondi, A Bismark, K Boese, A Brown, G Bruno, R Budnik, C Cai, C Capelli, J M R Cardoso, A P Cimental Chávez, A P Colijn, J Conrad, J J Cuenca-García, V D'Andrea, L C Daniel Garcia, M P Decowski, A Deisting, C Di Donato, P Di Gangi, S Diglio, K Eitel, S El Morabit, A Elykov, A D Ferella, C Ferrari, H Fischer, T Flehmke, M Flierman, W Fulgione, C Fuselli, P Gaemers, R Gaior, M Galloway, F Gao, S Ghosh, R Giacomobono, R Glade-Beucke, L Grandi, J Grigat, H Guan, M Guida, P Gyorgy, R Hammann, A Higuera, C Hils, L Hoetzsch, N F Hood, M Iacovacci, Y Itow, J Jakob, F Joerg, Y Kaminaga, M Kara, P Kavrigin, S Kazama, M Kobayashi, D Koke, A Kopec, H Landsman, R F Lang, L Levinson, I Li, S Li, S Liang, Y-T Lin, S Lindemann, M Lindner, K Liu, M Liu, J Loizeau, F Lombardi, J Long, J A M Lopes, T Luce, Y Ma, C Macolino, J Mahlstedt, A Mancuso, L Manenti, F Marignetti, T Marrodán Undagoitia, K Martens, J Masbou, E Masson, S Mastroianni, A Melchiorre, J Merz, M Messina, A Michael, K Miuchi, A Molinario, S Moriyama, K Morå, Y Mosbacher, M Murra, J Müller, K Ni, U Oberlack, B Paetsch, Y Pan, Q Pellegrini, R Peres, C Peters, J Pienaar, M Pierre, G Plante, T R Pollmann, L Principe, J Qi, J Qin, D Ramírez García, M Rajado, R Singh, L Sanchez, J M F Dos Santos, I Sarnoff, G Sartorelli, J Schreiner, P Schulte, H Schulze Eißing, M Schumann, L Scotto Lavina, M Selvi, F Semeria, P Shagin, S Shi, J Shi, M Silva, H Simgen, C Szyszka, A Takeda, P-L Tan, D Thers, F Toschi, G Trinchero, C D Tunnell, F Tönnies, K Valerius, S Vecchi, S Vetter, F I Villazon Solar, G Volta, C Weinheimer, M Weiss, D Wenz, C Wittweg, V H S Wu, Y Xing, D Xu, Z Xu, M Yamashita, L Yang, J Ye, L Yuan, G Zavattini, M Zhong\",\"doi\":\"10.1103/PhysRevLett.134.111802\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p><p>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.</p>\",\"PeriodicalId\":20069,\"journal\":{\"name\":\"Physical review letters\",\"volume\":\"134 11\",\"pages\":\"111802\"},\"PeriodicalIF\":8.1000,\"publicationDate\":\"2025-03-21\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physical review letters\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1103/PhysRevLett.134.111802\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, MULTIDISCIPLINARY\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical review letters","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/PhysRevLett.134.111802","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, MULTIDISCIPLINARY","Score":null,"Total":0}
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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Physical review letters(PRL)covers the full range of applied, fundamental, and interdisciplinary physics research topics:
General physics, including statistical and quantum mechanics and quantum information
Gravitation, astrophysics, and cosmology
Elementary particles and fields
Nuclear physics
Atomic, molecular, and optical physics
Nonlinear dynamics, fluid dynamics, and classical optics
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Condensed matter and materials physics
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