{"id":12398,"date":"2022-11-16T15:23:24","date_gmt":"2022-11-16T14:23:24","guid":{"rendered":"https:\/\/www.pi.infn.it\/?p=12398"},"modified":"2022-11-16T15:23:26","modified_gmt":"2022-11-16T14:23:26","slug":"everything-you-wanted-to-know-about-new-physics-and-core-collapse-supernovae-but-were-afraid-to-ask-andrea-caputo-cern","status":"publish","type":"post","link":"https:\/\/www.pi.infn.it\/?p=12398","title":{"rendered":"Everything you wanted to know about New Physics and Core-collapse Supernovae: but were afraid to ask (Andrea Caputo &#8211; CERN)"},"content":{"rendered":"\n<div><span style=\"font-family: Calibri,Helvetica,sans-serif,serif,EmojiFont\"><span style=\"color: black;font-size: medium\"><b>Abstract<\/b><\/span><span style=\"color: black;font-size: medium\">:\u00a0<\/span><span style=\"color: black;font-size: medium\">Core-collapse supernovae (CCSN) are efficient laboratories to explore physics beyond the standard model (SM). In particular, they have been used to put strong constraints on axion and axion like particles, and on many other motivated extensions of the SM.\u00a0<\/span><span style=\"color: black;font-size: medium\">In this talk I will first introduce the subject and then focus on some new results for muon-philic interactions. Finally, I will also describe a particular class of CCSNe, the Low Energy CCSNe, and show how they can be used as efficient beam dump experiments to severely constrain radiative particle decays.<\/span><span style=\"color: black;font-size: medium\">.<\/span><\/span><\/div>\n<div><span style=\"font-family: Calibri,Helvetica,sans-serif,serif,EmojiFont\">\u00a0<\/span><\/div>\n<div><span style=\"font-family: Calibri,Helvetica,sans-serif,serif,EmojiFont\"><span style=\"color: black;font-size: medium\">Il seminario si terr\u00e0 in presenza nella sala riunioni 131 e via zoom<\/span><span style=\"color: black;font-size: medium\"><b>\u00a0<\/b><\/span><span style=\"color: black;font-size: medium\">al seguente indirizzo:\u00a0<\/span><\/span><\/div>\n<div><span style=\"font-family: Calibri,Helvetica,sans-serif,serif,EmojiFont\"><a id=\"LPlnk34841\" href=\"https:\/\/es.sonicurlprotection-fra.com\/click?PV=2&amp;MSGID=202211152258081058599&amp;URLID=3&amp;ESV=10.0.18.7423&amp;IV=C8C5540416E166C8923D31B0A9E97172&amp;TT=1668553090274&amp;ESN=KohOW0snR2FWyTlR7vrxiXLE%2F2t9rHzSSihnz4%2Bb9V0%3D&amp;KV=1536961729280&amp;B64_ENCODED_URL=aHR0cHM6Ly9pbmZuLWl0Lnpvb20udXMvai84NDI2MTcyMTg3OD9wd2Q9TURaTmFHZEJVbGN2VVVKWGEycGhTSFpWWms1c2R6MDk&amp;HK=B00E81044D94A7F52747179EB80E44C874060921DD66F206B56F36AEE590AF62\" target=\"_blank\" rel=\"noopener noreferrer\"><span id=\"LPlnk34841\"><\/span><\/a><span style=\"color: #0099cc;font-family: Roboto,sans-serif,serif,EmojiFont;font-size: xx-small\"><span id=\"LPlnk34841\"><a id=\"LPlnk34841\" href=\"https:\/\/es.sonicurlprotection-fra.com\/click?PV=2&amp;MSGID=202211152258081058599&amp;URLID=2&amp;ESV=10.0.18.7423&amp;IV=27EBAAA98D1F8BB37EDF04F635FC3D52&amp;TT=1668553090273&amp;ESN=3bQ4%2FOc3YSfjcI%2Bceu1%2Fnyq5QE%2B1RBGTLEhTnPUG70o%3D&amp;KV=1536961729280&amp;B64_ENCODED_URL=aHR0cHM6Ly9pbmZuLWl0Lnpvb20udXMvai84NDI2MTcyMTg3OD9wd2Q9TURaTmFHZEJVbGN2VVVKWGEycGhTSFpWWms1c2R6MDk&amp;HK=01C1661417B865EFA2239B3EFCFE39DE60BD6C58B2F7E58CEAD5E604AC61A104\" target=\"_blank\" rel=\"noopener noreferrer\"><span style=\"font-size: medium\">https:\/\/infn-it.zoom.us\/j\/84261721878?pwd=MDZNaGdBUlcvUUJXa2phSHZVZk5sdz09<\/span><\/a><a id=\"LPlnk34841\" href=\"https:\/\/infn-it.zoom.us\/j\/84261721878?pwd=MDZNaGdBUlcvUUJXa2phSHZVZk5sdz09\" target=\"_blank\" rel=\"noopener noreferrer\"><\/a><\/span><\/span><\/span><\/div>\n<div>\u00a0<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Abstract:\u00a0Core-collapse supernovae (CCSN) are efficient laboratories to explore physics beyond the standard model (SM). In particular, they have been used to put strong constraints on axion and axion like particles, and on many other motivated extensions of the SM.\u00a0In this talk I will first introduce the subject and then focus on some new results for [&hellip;]<\/p>\n","protected":false},"author":26,"featured_media":12399,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"_links_to":"","_links_to_target":""},"categories":[8],"tags":[],"publishpress_future_action":{"enabled":false,"date":"2026-05-15 03:18:10","action":"change-status","newStatus":"draft","terms":[],"taxonomy":"category"},"_links":{"self":[{"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/posts\/12398"}],"collection":[{"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/users\/26"}],"replies":[{"embeddable":true,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=12398"}],"version-history":[{"count":1,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/posts\/12398\/revisions"}],"predecessor-version":[{"id":12400,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/posts\/12398\/revisions\/12400"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=\/wp\/v2\/media\/12399"}],"wp:attachment":[{"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=12398"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=12398"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.pi.infn.it\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=12398"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}