{"id":1697,"date":"2022-11-30T16:16:24","date_gmt":"2022-11-30T15:16:24","guid":{"rendered":"https:\/\/www.fe.infn.it\/cosmologia\/?page_id=1697"},"modified":"2025-07-12T12:43:53","modified_gmt":"2025-07-12T10:43:53","slug":"theses-masters-degree","status":"publish","type":"page","link":"https:\/\/www.fe.infn.it\/cosmologia\/?page_id=1697&lang=en","title":{"rendered":"Theses – Master’s Degree"},"content":{"rendered":"

Academic Year 2023\/2024<\/strong><\/span><\/p>\n

Valentina Genesini
Determination of the Reionization optical depth through a combined analysis of Planck and WMAP data<\/strong><\/span>
Advisor: Luca Pagano
Co-advisor: Giacomo Galloni<\/p>\n

Academic Year 2022\/2023<\/strong><\/span><\/p>\n

Thomas Lovo
Primordial cosmological perturbations in noncommutative spacetimes<\/strong><\/span>
Advisors: M. Lattanzi, L. Pagano
Co-advisor: Giulia Gubitosi<\/p>\n

Andrea Morelli
Using convolutional neural networks to extract cosmological parameters from CMB polarization maps<\/strong><\/span>
Advisor: Luca Pagano<\/p>\n

Ettore Mancinelli (Universit\u00e0 degli Studi di Perugia)
Calcolo dello spettro delle perturbazioni primordiali scalari (Computing the spectrum of primordial scalar perturbations)<\/strong><\/span>
Advisor: Nicola Tomassetti (Universit\u00e0 degli Studi di Perugia)
Co-advisors: Mario Ballardini, Alessandro Gruppuso<\/p>\n

Academic Year 2021\/2022<\/strong><\/span><\/p>\n

Giorgia Zagatti
Searching for signatures of new physics in the CMB: constraints on cosmic birefringence<\/strong><\/span>
Advisor: Paolo Natoli
Coadvisor: Luca Pagano<\/p>\n

Academic Year 2020\/2021<\/strong><\/span><\/p>\n

Arianna Rizzieri
Component separation for the microwave sky in view of next-generation cosmic microwave background experiments<\/strong><\/span>
Advisor: Massimiliano Lattanzi<\/p>\n

Enrico Occhiuto
Cosmological tests for an ultralight axion-like dark energy model<\/strong><\/span>
Advisor: Massimiliano Lattanzi<\/p>\n

Mauro San Giovanni
Cosmological implications of see-saw models of neutrino mass generation<\/strong><\/span>
Advisor: Massimiliano Lattanzi<\/p>\n

Academic Year 2019\/2020<\/strong><\/span><\/p>\n

Bianca De Caro
Measuring kinematic boost of cosmological backgrounds with future CMB satellite experiments<\/strong><\/span>
Advisor: Luca Pagano<\/p>\n

Nicolo’ Elia Raffuzzi
Impact of instrumental systematics on future Cosmic Microwave Background observations: half-wave plate non-idealities and the quest for V modes experiments<\/strong><\/span>
Advisor: Paolo Natoli
Coadvisor: Martina Gerbino<\/p>\n

Academic Year 2016\/2017<\/strong><\/span><\/p>\n

Nitya Dal Pra
Primordial black holes as dark matter: current constraints from cosmic microwave background temperature and polarization<\/strong><\/span>
Advisor: Paolo Natoli
Coadvisor: Massimiliano Lattanzi<\/p>\n

Academic Year 2013\/2014<\/strong><\/span><\/p>\n

Linda Polastri
CMB directional anomalies as seen by Planck<\/strong><\/span>
Advisor: Paolo Natoli
External advisor: Alessandro Gruppuso<\/p>\n

Academic Year 2012\/2013<\/strong><\/span><\/p>\n

Francesco Forastieri
Constraints on non-standard neutrino interactions from Planck 2013 CMB data<\/strong><\/span>
Advisor: Paolo Natoli
Coadvisor: Massimiliano Lattanzi<\/p>\n\n\n

<\/p>\n","protected":false},"excerpt":{"rendered":"

Academic Year 2023\/2024 Valentina GenesiniDetermination of the Reionization optical depth through a combined analysis of Planck and WMAP dataAdvisor: Luca PaganoCo-advisor: Giacomo Galloni Academic Year 2022\/2023 Thomas LovoPrimordial cosmological perturbations in noncommutative spacetimesAdvisors: M. Lattanzi, L. PaganoCo-advisor: Giulia Gubitosi Andrea MorelliUsing convolutional neural networks to extract cosmological parameters from CMB polarization mapsAdvisor: Luca Pagano Ettore […]<\/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-1697","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages\/1697","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=1697"}],"version-history":[{"count":8,"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages\/1697\/revisions"}],"predecessor-version":[{"id":2386,"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=\/wp\/v2\/pages\/1697\/revisions\/2386"}],"wp:attachment":[{"href":"https:\/\/www.fe.infn.it\/cosmologia\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1697"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}