Orateur
Massimiliano Lattanzi
(Istituto Nazionale di Fisica Nucleare)
Description
In this talk I will discuss how observations of the cosmic microwave background and of cosmological large-scale structures can be used to constrain the properties of neutrinos and other light relics. I will focus on "new physics" scenarios (e.g. beyond-standard-model neutrino interactions, axion-like particles....). I will further discuss detection prospects from forthcoming cosmological observations.
Auteur principal
Massimiliano Lattanzi
(Istituto Nazionale di Fisica Nucleare)
