{"id":241,"date":"2021-01-22T13:24:00","date_gmt":"2021-01-22T12:24:00","guid":{"rendered":"https:\/\/web.infn.it\/strings\/?p=241"},"modified":"2021-02-25T16:54:34","modified_gmt":"2021-02-25T15:54:34","slug":"seminar-february-11-n-gaddam","status":"publish","type":"post","link":"https:\/\/web.infn.it\/strings\/seminar-february-11-n-gaddam\/","title":{"rendered":"Seminar February 11: N. Gaddam"},"content":{"rendered":"\n<p>On February 11 we will have a seminar by<\/p>\n\n\n\n<p><strong>Nava Gaddam<\/strong> (Utrecht)<\/p>\n\n\n\n<p><strong>Title<\/strong>: The black hole eikonal and the information paradox<\/p>\n\n\n\n<p><strong>Abstract<\/strong>: In this talk, I will show that there is a remarkable phase of quantum gravity (which we will call the &#8216;black hole eikonal&#8217; phase) where gravitational collision energies near the horizon satisfy E &gt;&gt; \\gamma M_Pl, with \\gamma = M_Pl\/M_BH. I will argue that this regime captures gravitational scattering with impact parameters smaller than the Schwarzschild radius. Scattering amplitudes are unitary suggesting a resolution of the information paradox; I will sketch the explicit derivation of the 2-2 amplitude&nbsp;for massless scalars, non-perturbatively in \\gamma. Owing to the low energies of collisions, there are no firewalls experienced by infalling observers. A consequence of these results is that the information paradox is an emergent one at low energies and does not require detailed ultra-violet physics for a resolution.&nbsp;<\/p>\n\n\n\n<p>Meeting information:<br><strong>11th of February 14:30 Italian Time<br>Zoom Meeting <a href=\"https:\/\/zoom.us\/j\/198435430\">https:\/\/zoom.us\/j\/19843543<\/a><\/strong><\/p>\n\n\n\n<p>You can watch the recording at<br><a href=\"https:\/\/pandora.infn.it\/public\/be3ca2\">https:\/\/pandora.infn.it\/public\/be3ca2<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>On February 11 we will have a seminar by Nava Gaddam (Utrecht) Title: The black hole eikonal and the information paradox Abstract: In this talk, I will show that there is a remarkable phase of quantum gravity (which we will call the &#8216;black hole eikonal&#8217; phase) where gravitational collision energies near the horizon satisfy E &hellip; <a href=\"https:\/\/web.infn.it\/strings\/seminar-february-11-n-gaddam\/\" class=\"more-link\">Continue reading<span class=\"screen-reader-text\"> &#8220;Seminar February 11: N. Gaddam&#8221;<\/span><\/a><\/p>\n","protected":false},"author":5,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[8],"tags":[],"class_list":["post-241","post","type-post","status-publish","format-standard","hentry","category-seminar"],"_links":{"self":[{"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/posts\/241","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/comments?post=241"}],"version-history":[{"count":4,"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/posts\/241\/revisions"}],"predecessor-version":[{"id":255,"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/posts\/241\/revisions\/255"}],"wp:attachment":[{"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/media?parent=241"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/categories?post=241"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/web.infn.it\/strings\/wp-json\/wp\/v2\/tags?post=241"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}