{"id":3219,"date":"2024-07-11T09:00:15","date_gmt":"2024-07-11T00:00:15","guid":{"rendered":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?p=3219"},"modified":"2024-07-11T08:17:46","modified_gmt":"2024-07-10T23:17:46","slug":"first-measurement-of-a-nuclear-recoil-signal-from-solar-neutrinos-with-xenonnt","status":"publish","type":"post","link":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/blog\/2024\/07\/11\/3219\/","title":{"rendered":"First measurement of a nuclear recoil signal from solar neutrinos with XENONnT"},"content":{"rendered":"
\"\"
Inside the TPC of the XENONnT detector (credit: XENON Collaboration)<\/figcaption><\/figure>\n

The XENON collaboration is an international collaboration between the United States, Europe and Japan, involving the KMI and ISEE at the Nagoya University, the Kavli IPMU, WPI at the University of Tokyo, the Institute for Cosmic Ray Research at the University of Tokyo and Kobe University. The collaboration has observed for the first time the scattering of neutrinos and xenon nuclei produced by the Sun in the XENONnT experiment, a dark matter search experiment currently in operation. The results were reported at the international conference IDM2024 in L’Aquila, Italy, on 10 July (Japan time).<\/p>\n

Please refer to XENON Collaboration<\/a> for details.<\/p>\n","protected":false},"excerpt":{"rendered":"

The XENON collaboration is an international collaboration between the United States, Europe and Japan, involving the KMI and ISEE at the Nagoya University, the Kavli IPMU, WPI at the University of Tokyo, the Institute for Cosmic Ray Research at the University of Tokyo and Kobe University. The collaboration has observed for the first time the scattering of neutrinos and xenon nuclei produced by the Sun in the XENONnT experiment, a dark matter search experiment currently in operation. The results were … <\/p>\n","protected":false},"author":17,"featured_media":3221,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":""},"categories":[61],"tags":[],"acf":[],"yoast_head":"\nFirst measurement of a nuclear recoil signal from solar neutrinos with XENONnT - KMI - Nagoya University<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/blog\/2024\/07\/11\/3219\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"First measurement of a nuclear recoil signal from solar neutrinos with XENONnT - KMI - Nagoya University\" \/>\n<meta property=\"og:description\" content=\"The XENON collaboration is an international collaboration between the United States, Europe and Japan, involving the KMI and ISEE at the Nagoya University, the Kavli IPMU, WPI at the University of Tokyo, the Institute for Cosmic Ray Research at the University of Tokyo and Kobe University. The collaboration has observed for the first time the scattering of neutrinos and xenon nuclei produced by the Sun in the XENONnT experiment, a dark matter search experiment currently in operation. 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