{"id":38012,"date":"2020-05-29T18:07:54","date_gmt":"2020-05-29T16:07:54","guid":{"rendered":"\/gruppo2\/?page_id=38012"},"modified":"2024-01-31T16:25:38","modified_gmt":"2024-01-31T15:25:38","slug":"thesis-opportunities","status":"publish","type":"page","link":"\/gruppo2\/en\/thesis-opportunities\/","title":{"rendered":"Thesis Opportunities"},"content":{"rendered":"\n<h1 class=\"has-text-align-center wp-block-heading\"><span style=\"color:#007BB3\" class=\"tadv-color\">Thesis Opportunities<\/span><\/h1>\n\n\n\n<p style=\"text-align: left;\"><span class=\"collapseomatic noarrow\" id=\"Neutrino_Physics\"  tabindex=\"0\" alt=\"Information about Neutrino Physics\" title=\"Information about Neutrino Physics\"    ><strong>+ Neutrino Physics<\/strong><\/span><span id='swap-Neutrino_Physics'  class='colomat-swap' style='display:none;'><strong>- Neutrino Physics<\/strong><\/span><div id=\"target-Neutrino_Physics\" class=\"collapseomatic_content \">\n<p style=\"text-align: center;\"><span style=\"color: #007bb3; font-family: Open Sans;\"><strong>Neutrino Physics<\/strong><\/span><\/p>\n<p>CUORE<\/p>\n<p>&#8220;Analysis of the vibration modes of cryogenic detectors in correlation with an associated seismometric system for the determination of the transfer function of vibrational noise of seismic and \/ or anthropic origin to the bolometric crystals of the CUORE experiment&#8221;.<\/p>\n<p><em>Keywords<\/em>: master&#8217;s degree, experimental thesis, data analysis, background noise reduction, seismometers<br \/><em>Duration of the thesis<\/em>: about six months.<\/p>\n<p>The thesis will involve, compatibly with the Covid-19 health situation, short periods of activity at the INFN Gran Sasso National Laboratories and will take place in collaboration with american colleagues.<\/p>\n<p>CUPID<\/p>\n<p>&#8220;Optimization of neutron transmuted doped ( NTD ) temperature transducers for the new generation of experiments with selenium molybdate bolometric detectors, CUPID experiment.&#8221;<\/p>\n<p><em>Keywords<\/em>: master\u2019s degree, experimental thesis, research and development and detectors construction, solid state, silicon and germanium, detectors.<br \/><em>Duration of the thesis<\/em>: about six months.<br \/>The thesis will involve, compatibly with the Covid-19 health situation, short periods of activity at the INFN Gran Sasso National Laboratories and will take place in collaboration with American colleagues<br \/>The activity will also take place in collaboration with the Bologna Unit of the Italian National Research Council (CNR) Institute for Microelectronics and Microsystems (IMM).<\/p>\n<p>ENUBET<\/p>\n<p>\u00a0<\/p>\n<\/div>\n\n\n\n<span class=\"collapseomatic noarrow\" id=\"Radiation_from_the_Universe\"  tabindex=\"0\" alt=\"Information about Radiation from the Universe\" title=\"Information about Radiation from the Universe\"    ><strong>+ Radiation from the Universe<\/strong><\/span><span id='swap-Radiation_from_the_Universe'  class='colomat-swap' style='display:none;'><strong>- Radiation from the Universe<\/strong><\/span><div id=\"target-Radiation_from_the_Universe\" class=\"collapseomatic_content \">\n<p style=\"text-align: center;\"><span style=\"font-family: Open Sans; color: #007bb3;\"><strong>Radiation from the Universe<\/strong><\/span><\/p>\n<p>AMS<\/p>\n<div id=\"tw-target-text-container\" class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\">The Alpha Magnetic Spectrometer (AMS) is a high energy physics experiment in space. It measures cosmic rays (CRs), which are high energy particles and nuclei coming from outer space. <br \/>AMS has been installed aboard the International Space Station in 2011, and has collected more than 160 billion CRs, as of October 2020. <br \/>The main purposes of the experiment are:<\/div>\n<div>\u00a0<\/div>\n<ol style=\"list-style-type: lower-alpha;\">\n<li class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\">the understanding of the matter\/anti-matter asymmetry in the universe through the direct search of complex anti-matter in space;<\/li>\n<li class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\">indirect search of dark matter in CRs;<\/li>\n<li class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\">the understanding of the origin, acceleration, and propagation of CRs;<\/li>\n<li class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\">\u00a0study of the heliosphere and of the Earth magnetosphere \u00a0 (space weather, solar modulation of cosmic rays, &#8230;).<\/li>\n<\/ol>\n<div class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\"><br \/>AMS Bologna group is deeply involved in the AMS data analysis. <br \/>In parallel, the group is also helping the development of CRs models that describe the propagation of CRs in the galaxy (GALPROP) and in the heliosphere (HelMod).<\/div>\n<div class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\"><br \/>We will propose to students the use of official AMS data. The research topic will be agreed upon among the research lines stated above. In the case of master thesis or Ph.D. students, training periods at the AMS control center located in CERN (European Organization for Nuclear Research) in Geneva, or at the ASI (Agenzia Spaziale Italiana) in Rome will be planned.<\/div>\n<div class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: justify;\"><br \/>Contacts: <a class=\"moz-txt-link-abbreviated\" href=\"mailto:andrea.contin@bo.infn.it\">andrea.contin@bo.infn.it<\/a>, <a class=\"moz-txt-link-abbreviated\" href=\"mailto:nicolo.masi@bo.infn.it\">nicolo.masi@bo.infn.it<\/a> and <br \/>\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0\u00a0 <a class=\"moz-txt-link-abbreviated\" href=\"mailto:alberto.oliva@bo.infn.it\">alberto.oliva@bo.infn.it<\/a><\/div>\n<div>\u00a0<\/div>\n<div class=\"tw-ta-container hide-focus-ring tw-nfl\" style=\"text-align: left;\">For more information about the experiment please visit: <a class=\"moz-txt-link-freetext\" href=\"https:\/\/ams02.space\/\" data-wpel-link=\"external\" target=\"_blank\" rel=\"nofollow external noopener noreferrer\" title=\"Open page in new tab https:\/\/ams02.space\/\">https:\/\/ams02.space\/<\/a><\/div>\n<div id=\"tw-target-rmn-container\" class=\"tw-ta-container hide-focus-ring tw-nfl\">\n<pre id=\"tw-target-rmn\" class=\"tw-data-placeholder tw-text-small tw-ta\" data-placeholder=\"\">\u00a0<\/pre>\n<\/div>\n<p>ANTARES\/KM3NeT<\/p>\n<p>Neutrino telescope group offers several opportunities for bachelor, master and PhD theses on different research subjects:<\/p>\n<ul style=\"list-style-type: square;\">\n<li>analysis of ANTARES e KM3NeT data to search for neutrino sources and in coincidence with gravitational waves,\u00a0 Gamma Ray Burst and other events according to a multimessenger approach.<\/li>\n<li>use of neural networks and Machine Learning strategies to discriminate among different patterns in event reconstructions for ANTARES and KM3NeT telescopes.<\/li>\n<li>implementation of the KM3NeT data acquisition system.<\/li>\n<\/ul>\n<p>These activities are carried on in strict coordination with European and extra-European scientific institutions and universities.<\/p>\n<p>LIMADOU<\/p>\n<\/div>\n<p>\u00a0<\/p>\n\n\n\n<span class=\"collapseomatic noarrow\" id=\"Dark_Universe\"  tabindex=\"0\" alt=\"Information about Dark Universe\" title=\"Information about Dark Universe\"    ><strong>+ Dark Universe<\/strong><\/span><span id='swap-Dark_Universe'  class='colomat-swap' style='display:none;'><strong>- Dark Universe<\/strong><\/span><div id=\"target-Dark_Universe\" class=\"collapseomatic_content \">\n<p style=\"text-align: center;\"><span style=\"font-family: Open Sans; color: #007bb3;\"><strong>Dark Universe<\/strong><\/span><\/p>\n<p>DARKSIDE<\/p>\n<p>The <a href=\"\/gruppo2\/en\/darkside-en\/\" data-wpel-link=\"internal\" target=\"_self\" rel=\"nofollow noopener noreferrer\" title=\"Open page DarkSide Bologna\">DarkSide Bologna<\/a> group offers the opportunity to carry out three-year and master&#8217;s theses related to the development, construction and test of the signal transmission system from the photodetectors (SiPM) to the read-out electronics, as well as to the assembly and characterisation of the photodetectors that will be used. in the experiment. The activities include cryogenic and clean room tests in Bologna and participation to tests at the Gran Sasso National Laboratories and\/or at CERN.<\/p>\n<p>EUCLID<\/p>\n<p>The topics here listed can be developed at different levels, as Master thesis or PhD thesis.<\/p>\n<ul>\n<li>Analysis of Euclid NISP Spectroscopic data: from raw data to the study of cosmological parameters<\/li>\n<li>Constraints on neutrino properties with Euclid<\/li>\n<\/ul>\n<p>XENON<\/p>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Thesis Opportunities \u00a0<\/p>\n","protected":false},"author":35,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"template-page-builder-no-sidebar.php","meta":{"_lmt_disableupdate":"no","_lmt_disable":"","footnotes":""},"class_list":["post-38012","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"\/gruppo2\/wp-json\/wp\/v2\/pages\/38012","targetHints":{"allow":["GET"]}}],"collection":[{"href":"\/gruppo2\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"\/gruppo2\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"\/gruppo2\/wp-json\/wp\/v2\/users\/35"}],"replies":[{"embeddable":true,"href":"\/gruppo2\/wp-json\/wp\/v2\/comments?post=38012"}],"version-history":[{"count":32,"href":"\/gruppo2\/wp-json\/wp\/v2\/pages\/38012\/revisions"}],"predecessor-version":[{"id":38804,"href":"\/gruppo2\/wp-json\/wp\/v2\/pages\/38012\/revisions\/38804"}],"wp:attachment":[{"href":"\/gruppo2\/wp-json\/wp\/v2\/media?parent=38012"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}