{"id":2141,"date":"2023-12-14T14:03:24","date_gmt":"2023-12-14T13:03:24","guid":{"rendered":"https:\/\/www.fe.infn.it\/cosmologia\/?page_id=2141"},"modified":"2025-07-11T13:59:33","modified_gmt":"2025-07-11T11:59:33","slug":"antonio-raffaelli-en","status":"publish","type":"page","link":"https:\/\/www.fe.infn.it\/cosmologia\/?page_id=2141&lang=en","title":{"rendered":"Antonio Raffaelli"},"content":{"rendered":"<h1><span style=\"color: #22a1c4;\"><strong>Antonio Raffaelli<\/strong><\/span><\/h1>\n<p>PhD student<\/p>\n<h4><span style=\"color: #ffffff;\"><strong>XXXIX cycle<\/strong><\/span><\/h4>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-1242 size-medium\" src=\"http:\/\/www.fe.infn.it\/cosmologia\/wp-content\/uploads\/2024\/01\/foto_bio.png\" alt=\"Antonio Raffaelli\" width=\"234\" height=\"300\"><\/p>\n<p>Antonio&#8217;s research focuses on the study of methods for reconstructing the spectrum of primordial perturbations from measurements of the cosmic microwave background, in temperature and polarization, and measurements of the large-scale distribution of structures. The study is also applied to particular parameterizations of primordial features, with deviations from a primordial spectrum described by a power law, associated with anomalies observed in measurements of fluctuations in temperature of the cosmic microwave background. In his master&#8217;s thesis work, Antonio studied anisotropies in the cosmic neutrino background and their cross-correlation with anisotropies in temperature of the cosmic background radiation.<\/p>\n<p><em><strong>Contacts:<\/strong><\/em><\/p>\n<p>E-mail: <a href=\"mailto:antonio.raffaelli@unife.it\">antonio.raffaelli@unife.it<\/a><\/p>\n<p>Office: Building C, room 427<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Antonio Raffaelli PhD student XXXIX cycle Antonio&#8217;s research focuses on the study of methods for reconstructing the spectrum of primordial perturbations from measurements of the cosmic microwave background, in temperature and polarization, and measurements of the large-scale distribution of structures. The study is also applied to particular parameterizations of primordial features, with deviations from a [&hellip;]<\/p>\n","protected":false},"author":4,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-2141","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages\/2141","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/users\/4"}],"replies":[{"embeddable":true,"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=2141"}],"version-history":[{"count":4,"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages\/2141\/revisions"}],"predecessor-version":[{"id":2289,"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages\/2141\/revisions\/2289"}],"wp:attachment":[{"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2141"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}