{"id":1184,"date":"2018-12-17T13:41:59","date_gmt":"2018-12-17T04:41:59","guid":{"rendered":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?post_type=seminar&#038;p=1184"},"modified":"2021-07-30T12:35:38","modified_gmt":"2021-07-30T03:35:38","slug":"exploring-physics-of-neutron-star-matter-with-gravitational-waves-from-neutron-star-merger","status":"publish","type":"seminar","link":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/1184\/","title":{"rendered":"Exploring physics of neutron star matter with gravitational waves from neutron star merger"},"content":{"rendered":"<div class=\"title\">\n<div class=\"title\"><strong><span style=\"font-size: 14pt;\"><span class=\"paren\" id=\"left\">&#8220;<\/span>Exploring physics of neutron star matter with gravitational waves from neutron star merger<span class=\"paren\" id=\"right\">&#8220;<\/span><\/span><\/strong><\/div>\n<div class=\"person\">\n<div class=\"speaker\"><strong><span style=\"font-size: 14pt;\"><br \/>\n<\/span><\/strong><span style=\"font-size: 14pt;\"><span style=\"font-size: 12pt;\">Yuichiro Sekiguchi<\/span><\/span><span class=\"paren\" id=\"left\">(<\/span>Department of Physics, Toho University<span class=\"paren\" id=\"right\">)<\/span><\/div>\n<\/div>\n<div class=\"date\">January 30, 2019 (Wed) 17:00-<\/div>\n<div class=\"place\">KMI Science Symposia (ES635)<\/p>\n<\/div>\n<div class=\"abstract\"><strong>Abstract<span class=\"delimiter\">:<\/span><\/strong><\/p>\n<div class=\"page\" title=\"Page 1\">\n<div class=\"section\">\n<div class=\"layoutArea\">\n<div class=\"column\">\n<p><span>Neutron stars provide us a unique laboratory for studying the physics of\u00a0<\/span>nuclear\/hadronic matter. In particular, a merger event of binary neutron stars can be regarded as a cosmological collider experiment. With this ragard, there are a number of theoretical studies of constraining the equation of state of neutron star matter using gravitational wave (GW) from neutron star mergers. Then, In the spectacular event of GW170817, information of the equation of state are extracted from GW. The theoretical basis and recent progress, as well as future prospects of this research field will be presented and discussed.<\/p>\n<p>&nbsp;<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"attach\">\n<div class=\"attach-ent\"><a href=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/KMI-colloquium_Sekiguchi_20190130.pdf\"><img decoding=\"async\" src=\"https:\/\/www.kmi.nagoya-u.ac.jp\/images\/btn\/file.gif\" alt=\"[file]\" \/><\/a><span>\u00a0<\/span>Poster<\/div>\n<\/div>\n<\/div>\n","protected":false},"featured_media":0,"template":"","tags":[],"seminar_category":[55],"acf":{"s_now_accepting":true,"s_date_order":"2019-01-30 17:00:00","s_date_end":null,"s_date_text":"2019-01-30 5PM","s_text":"Yuichiro Sekiguchi (Department of Physics, Toho 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>Exploring physics of neutron star matter with gravitational waves from neutron star merger - 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\/1184\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Exploring physics of neutron star matter with gravitational waves from neutron star merger - KMI - Nagoya University\" \/>\n<meta property=\"og:description\" content=\"&#8220;Exploring physics of neutron star matter with gravitational waves from neutron star merger&#8220; Yuichiro Sekiguchi(Department of Physics, Toho University) January 30, 2019 (Wed) 17:00- KMI Science Symposia (ES635) Abstract: Neutron stars provide us a unique laboratory for studying the physics of\u00a0nuclear\/hadronic matter. In particular, a merger event of binary neutron stars can be regarded as a cosmological collider experiment. 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