{"id":1182,"date":"2018-12-17T13:37:09","date_gmt":"2018-12-17T04:37:09","guid":{"rendered":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?post_type=seminar&#038;p=1182"},"modified":"2019-02-01T15:48:49","modified_gmt":"2019-02-01T06:48:49","slug":"direct-dark-matter-search-with-xenonnt","status":"publish","type":"seminar","link":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/","title":{"rendered":"Direct dark matter search with XENONnT"},"content":{"rendered":"<div class=\"title\"><span style=\"font-size: 18pt;\"><span class=\"paren\" id=\"left\">&#8220;<\/span>Direct dark matter search with XENONnT<span class=\"paren\" id=\"right\">&#8220;<\/span><\/span><\/div>\n<div class=\"person\">\n<div class=\"speaker\">Singo Kazama\u00a0<span class=\"paren\" id=\"left\">(<\/span>KMI, Nagoya University<span class=\"paren\" id=\"right\">)<\/span><\/div>\n<\/div>\n<div class=\"date\">December 12, 2018 (Wed) 17:30-<\/div>\n<div class=\"place\">KMI Science Symposia (ES635)<\/div>\n<div><\/div>\n<div class=\"abstract\"><strong>Abstract<span class=\"delimiter\">:<\/span><\/strong><\/p>\n<p>The XENON series of experiments has been highly successful in pushing the limits of WIMP direct searches for more than a decade. We are currently operating the XENON1T detector, the most sensitive dark matter detector ever built, at Laboratori Nazionali del Gran Sasso (LNGS). The XENON1T experimental setup and infrastructure were designed to allow for a fast upgrade of its central detector, a two-phase xenon Time Projection Chamber (TPC). The XENONnT project, the next phase of the program, will feature a new TPC with an active target of ~6 tonnes of Xenon (4 tonne fiducial) and will implement a series of technological solutions aiming to further suppress the dominant background sources and boost the physics reach of the experiment. In this talk, an update on the status and prospects of the XENONnT phase (especially Japan&#8217;s contribution to the experiment) will be presented.<\/p>\n<\/div>\n","protected":false},"featured_media":0,"template":"","tags":[],"seminar_category":[58],"acf":{"s_now_accepting":true,"s_date_order":"2018-12-12 17:30:00","s_date_end":null,"s_date_text":"2018-12-12 5:30PM","s_text":"Singo Kazama (KMI, Nagoya University)","s_place":"KMI Science Symposia (ES635)","s_place_other":"","s_categoryother":"","s_poster":"","s_poster2":"","s_slide":""},"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v23.5 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>Direct dark matter search 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\/seminar\/1182\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Direct dark matter search with XENONnT - KMI - Nagoya University\" \/>\n<meta property=\"og:description\" content=\"&#8220;Direct dark matter search with XENONnT&#8220; Singo Kazama\u00a0(KMI, Nagoya University) December 12, 2018 (Wed) 17:30- KMI Science Symposia (ES635) Abstract: The XENON series of experiments has been highly successful in pushing the limits of WIMP direct searches for more than a decade. We are currently operating the XENON1T detector, the most sensitive dark matter detector ever built, at Laboratori Nazionali del Gran Sasso (LNGS). The XENON1T experimental setup and infrastructure were designed to allow for a fast upgrade of its &hellip;\" \/>\n<meta property=\"og:url\" content=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/\" \/>\n<meta property=\"og:site_name\" content=\"KMI - Nagoya University\" \/>\n<meta property=\"article:modified_time\" content=\"2019-02-01T06:48:49+00:00\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data1\" content=\"1 minute\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\/\/schema.org\",\"@graph\":[{\"@type\":\"WebPage\",\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/\",\"url\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/\",\"name\":\"Direct dark matter search with XENONnT - KMI - Nagoya University\",\"isPartOf\":{\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/#website\"},\"datePublished\":\"2018-12-17T04:37:09+00:00\",\"dateModified\":\"2019-02-01T06:48:49+00:00\",\"breadcrumb\":{\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/#breadcrumb\"},\"inLanguage\":\"en-US\",\"potentialAction\":[{\"@type\":\"ReadAction\",\"target\":[\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/\"]}]},{\"@type\":\"BreadcrumbList\",\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/#breadcrumb\",\"itemListElement\":[{\"@type\":\"ListItem\",\"position\":1,\"name\":\"Home\",\"item\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/\"},{\"@type\":\"ListItem\",\"position\":2,\"name\":\"Seminars\",\"item\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/\"},{\"@type\":\"ListItem\",\"position\":3,\"name\":\"Direct dark matter search with XENONnT\"}]},{\"@type\":\"WebSite\",\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/#website\",\"url\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/\",\"name\":\"KMI - Nagoya University\",\"description\":\"Nagoya University: Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI)\",\"potentialAction\":[{\"@type\":\"SearchAction\",\"target\":{\"@type\":\"EntryPoint\",\"urlTemplate\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?s={search_term_string}\"},\"query-input\":{\"@type\":\"PropertyValueSpecification\",\"valueRequired\":true,\"valueName\":\"search_term_string\"}}],\"inLanguage\":\"en-US\"}]}<\/script>\n<!-- \/ Yoast SEO plugin. -->","yoast_head_json":{"title":"Direct dark matter search with XENONnT - KMI - Nagoya University","robots":{"index":"index","follow":"follow","max-snippet":"max-snippet:-1","max-image-preview":"max-image-preview:large","max-video-preview":"max-video-preview:-1"},"canonical":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1182\/","og_locale":"en_US","og_type":"article","og_title":"Direct dark matter search with XENONnT - KMI - Nagoya University","og_description":"&#8220;Direct dark matter search with XENONnT&#8220; Singo Kazama\u00a0(KMI, Nagoya University) December 12, 2018 (Wed) 17:30- KMI Science Symposia (ES635) Abstract: The XENON series of experiments has been highly successful in pushing the limits of WIMP direct searches for more than a decade. 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