Obiettivo The purpose of this cosmology project is to study the content and evolution of our Universe using the distribution of matter on large scales. A key goal of forthcoming galaxy surveys is probing fundamental physics, such as the mass of neutrinos and the nature of dark energy, the component sourcing cosmic acceleration. The analysis and interpretation of their data crucially relies on the development of perturbation theory methods and other theoretical tools to describe and predict the evolution of large scale structures in the universe, particularly in the non-linear regime. This project aims to establish the optimal approach to compute the growth of structures and to extract information about dark energy and neutrino masses from the data.This action will address important questions in non-linear structure formation. More specifically, I will 1) devise efficient techniques to obtain information on non-linear clustering from data and apply it to bispectrum estimators and BAO reconstruction; 2) obtain the predictions for general massive neutrinos and dark energy models, beyond the power spectrum; and 3) improve the precision of semi-analytical methods to compute non-linear perturbations on small scales; A very concrete goal of the project is to produce a numerical code and make it public. This code will find direct application in the forecast and analysis of the data from the Euclid mission and other galaxy surveys, to probe the properties of neutrinos and the nature of gravity.In the outgoing phase I will work at University of California, Berkeley (US) to benefit from its great involvement in galaxy surveys and expertise in studies of large scale structure in connection to observations. In the return phase I will work in the Institut de Physique Théorique Saclay (France) where many theoretical developments in perturbation theory and extensions to non-standard models have been developed. Campo scientifico natural sciencesphysical sciencestheoretical physicsparticle physicsneutrinosnatural sciencesphysical sciencesastronomyobservational astronomygravitational wavesnatural sciencesphysical sciencesastronomyastrophysicsblack holesnatural sciencesphysical sciencesastronomyastrophysicsdark matternatural sciencesphysical sciencesastronomyphysical cosmology Parole chiave Cosmology dark energy modified gravity perturbation theory non-linear effects large scale structure of the Universe galaxy surveys bispectrum gravitation Programma(i) H2020-EU.1.3. - EXCELLENT SCIENCE - Marie Skłodowska-Curie Actions Main Programme H2020-EU.1.3.2. - Nurturing excellence by means of cross-border and cross-sector mobility Argomento(i) MSCA-IF-2015-GF - Marie Skłodowska-Curie Individual Fellowships (IF-GF) Invito a presentare proposte H2020-MSCA-IF-2015 Vedi altri progetti per questo bando Meccanismo di finanziamento MSCA-IF - Marie Skłodowska-Curie Individual Fellowships (IF) Coordinatore COMMISSARIAT A L ENERGIE ATOMIQUE ET AUX ENERGIES ALTERNATIVES Contribution nette de l'UE € 264 668,40 Indirizzo RUE LEBLANC 25 75015 PARIS 15 Francia Mostra sulla mappa Regione Ile-de-France Ile-de-France Paris Tipo di attività Research Organisations Collegamenti Contatta l’organizzazione Opens in new window Sito web Opens in new window Partecipazione a programmi di R&I dell'UE Opens in new window Rete di collaborazione HORIZON Opens in new window Costo totale € 264 668,40 Partner (1) Classifica in ordine alfabetico Classifica per Contributo netto dell'UE Espandi tutto Riduci tutto Partner Le organizzazioni partner contribuiscono all’attuazione dell’azione, ma non sottoscrivono l’accordo di sovvenzione. THE REGENTS OF THE UNIVERSITY OF CALIFORNIA Stati Uniti Contribution nette de l'UE € 0,00 Indirizzo FRANKLIN STREET 1111 12 FLOOR 94607 OAKLAND CA Mostra sulla mappa Tipo di attività Higher or Secondary Education Establishments Collegamenti Contatta l’organizzazione Opens in new window Sito web Opens in new window Partecipazione a programmi di R&I dell'UE Opens in new window Rete di collaborazione HORIZON Opens in new window Costo totale € 172 130,40
