{"id":2187,"date":"2020-08-31T10:30:18","date_gmt":"2020-08-31T01:30:18","guid":{"rendered":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?post_type=seminar&#038;p=2187"},"modified":"2021-07-13T11:24:25","modified_gmt":"2021-07-13T02:24:25","slug":"mysterious-fast-radio-bursts-and-implication-from-magnetars-to-their-origins","status":"publish","type":"seminar","link":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2187\/","title":{"rendered":"Mysterious fast radio bursts and implication from magnetars to their origins"},"content":{"rendered":"<p><span style=\"font-size: 14pt;background-color: #99ccff\"><strong>\u00a0&#8220;<span style=\"color: #333399;background-color: #99ccff\">KMI colloquium&#8221;\u00a0 \u00a0 30th September (Wed)\u00a0 <span style=\"color: #800000\">16:00<\/span>&#8211;<\/span><span style=\"color: #333399;background-color: #99ccff\"><br \/>\n<\/span><\/strong><\/span><\/p>\n<p><span style=\"font-size: 14pt\"><span style=\"color: #333399\"><span style=\"color: #333333\">Speaker<\/span> :Teruaki Enoto<br \/>\n<span style=\"font-size: 12pt\">(RIKEN, Extreme natural phenomema RIKEN Hakubi Research Team)<\/span><strong><br \/>\n<\/strong><\/span><\/span><span style=\"font-size: 14pt\"><span class=\"st\"><\/span><\/span><\/p>\n<p><span style=\"font-size: 14pt\"><span class=\"st\">Title : <\/span>Mysterious fast radio bursts and implication from magnetars to their origins<br \/>\n<img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/wp-content\/uploads\/sites\/2\/2020\/08\/Enoto-217x300.jpg\" alt=\"\" width=\"217\" height=\"300\" class=\"size-medium wp-image-2183 aligncenter\" srcset=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/wp-content\/uploads\/sites\/2\/2020\/08\/Enoto-217x300.jpg 217w, https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/wp-content\/uploads\/sites\/2\/2020\/08\/Enoto.jpg 628w\" sizes=\"(max-width: 217px) 100vw, 217px\" \/><br \/>\n<span style=\"font-size: 10pt\"><span class=\"st\"><span style=\"font-size: 14pt\">Poster :<a href=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/wp-content\/uploads\/sites\/2\/2020\/08\/Enoto__colloquium_2_20200930.pdf\">Enoto__colloquium_2_20200930<\/a><\/span><\/span><\/span><\/span><span style=\"font-size: 14pt\"><span style=\"font-size: 10pt\"><span class=\"st\"><br \/>\n<\/span><\/span><br \/>\n<\/span><span style=\"font-size: 12pt\">Abstract :In 2001, the Park observatory detected a mysterious radio spike with milliseconds&#8217; <br \/>\nduration\u00a0<\/span><span style=\"font-size: 12pt\">from the direction to the Magellanic cloud, which was called &#8220;Lorimer Burst&#8221; after its<br \/>\ndiscoverer. The number of similar radio transients has been gradually and later rapidly<br \/>\nincreased, and called &#8220;Fast Radio Bursts (FRBs).&#8221; The observational characteristics of FRBs<br \/>\nindicate the cosmological distance to its unknown sources. Now, the origin or origins of<br \/>\nFRBs have been actively studied by many astronomers. In 2020, an FRB event was<br \/>\ndiscovered during a bursting activity of a Galactic magnetar SGR 1935+2154. The magnetars<br \/>\nare a subgroup of neutron stars with the strongest magnetic field strength of ~10<span style=\"font-size: 8pt\"><sup>11<\/sup> <span style=\"font-size: 12pt\">T on its<\/span><br \/>\n<span style=\"font-size: 12pt\">stellar surface. They sometimes exhibit sporadic X-ray and soft gamma-ray burst emission<\/span><br \/>\n<span style=\"font-size: 12pt\">releasing stored magnetic energy. The recently discovered FRB association to SGR<\/span><br \/>\n<span style=\"font-size: 12pt\">1935+2154 indicates that magnetars are one promising candidate for FRBs&#8217; origin. At this<\/span><br \/>\n<span style=\"font-size: 12pt\">talk, I will review the story of rapidly developing fields of the FRBs and observational<\/span><br \/>\n<span style=\"font-size: 12pt\">implications from a diversity of neutron stars, especially magnetars, the strongest magnets of<\/span><br \/>\n<span style=\"font-size: 12pt\">our Universe.<\/span><br \/>\n<\/span><\/span><\/p>\n<p><span style=\"font-size: 14pt\"><\/span><span style=\"font-size: 12pt\"><\/span><\/p>\n<p><span style=\"font-size: 10pt\"><span class=\"st\">The colloquium will be held via ZOOM.<\/p>\n<p>\n<\/span><\/span><span class=\"st\" style=\"font-size: 10pt\"><\/span><\/p>\n<p>&nbsp;<\/p>\n","protected":false},"featured_media":0,"template":"","tags":[],"seminar_category":[55],"acf":{"s_now_accepting":true,"s_date_order":"2020-09-30 16:00:00","s_date_end":null,"s_date_text":"Wednesday,September 30th, 2020","s_text":"Teruaki Enoto (RIKEN, Extreme natural phenomema RIKEN Hakubi Research Team)","s_place":"zoom","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>Mysterious fast radio bursts and implication from magnetars to their origins - 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\/2187\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Mysterious fast radio bursts and implication from magnetars to their origins - KMI - Nagoya University\" \/>\n<meta property=\"og:description\" content=\"\u00a0&#8220;KMI colloquium&#8221;\u00a0 \u00a0 30th September (Wed)\u00a0 16:00&#8211; Speaker :Teruaki Enoto (RIKEN, Extreme natural phenomema RIKEN Hakubi Research Team) Title : Mysterious fast radio bursts and implication from magnetars to their origins Poster :Enoto__colloquium_2_20200930 Abstract :In 2001, the Park observatory detected a mysterious radio spike with milliseconds&#8217; duration\u00a0from the direction to the Magellanic cloud, which was called &#8220;Lorimer Burst&#8221; after its discoverer. 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