{"id":2561,"date":"2025-07-22T14:43:43","date_gmt":"2025-07-22T05:43:43","guid":{"rendered":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/?p=2561"},"modified":"2025-07-22T14:43:43","modified_gmt":"2025-07-22T05:43:43","slug":"2025-07-30","status":"publish","type":"post","link":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/2025\/07\/22\/2025-07-30\/","title":{"rendered":"2025-07-30"},"content":{"rendered":"\n<h2 class=\"wp-block-heading\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-bright-blue-color\">Supernova neutrinos in the multi-messenger era <\/mark><\/h2>\n\n\n\n<p class=\"has-text-align-right\">Speaker: Shunsaku Horiuchi (Science Tokyo)<\/p>\n\n\n\n<p>Abstract:<\/p>\n\n\n\n<p>The historical multi-messenger firework SN 1987A confirmed the importance of neutrinos in a core-collapse supernova. However, there have been no confirmed supernova neutrino detections in the three decades since, leaving many open questions unanswered. The rise of multi-messenger astronomy opens new opportunities to detect more of these precious messengers in the future. In this talk, I will start nearby, with new prospects from a supernova in the Milky Way galaxy, before moving further in distance, to distant galaxies that power an isotropic and constant diffuse flux of neutrinos. I will highlight how these offer complementary probes of core-collapse supernovae and associated phenomena. Along the way, I will cover how the combination of theoretical, observational astronomy, and experimental neutrino communities are crucial for progress in core-collapse supernovae in the multi-messenger era.\u00a0<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Supernova neutrinos in the multi-messenger era Speaker: Shunsaku Horiuchi (Science Tokyo) Abstract: The histor &hellip; <a href=\"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/2025\/07\/22\/2025-07-30\/\" class=\"more-link\"><span class=\"screen-reader-text\">&#8220;2025-07-30&#8221; \u306e<\/span>\u7d9a\u304d\u3092\u8aad\u3080<\/a><\/p>\n","protected":false},"author":31,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-2561","post","type-post","status-publish","format-standard","hentry","category-1"],"_links":{"self":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/2561","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/users\/31"}],"replies":[{"embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/comments?post=2561"}],"version-history":[{"count":1,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/2561\/revisions"}],"predecessor-version":[{"id":2562,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/posts\/2561\/revisions\/2562"}],"wp:attachment":[{"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/media?parent=2561"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/categories?post=2561"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/sci.nao.ac.jp\/seminars\/colloquium\/wp-json\/wp\/v2\/tags?post=2561"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}