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Magnetic fields are an ubiquitous presence in our Universe but a comprehensive theory describing their generation and evolution is still missing. An intriguing possibility is that these fields are generated in the pre-recombination Universe and then evolve passively until the epoch of structure formation. A clean way to prove the presence of primordial magnetic fields (PMF) is to look at Cosmic Microwave Background (CMB) anisotropies induced by these fields. In this talk, I will review the current and future bounds on PMFs as coming from the observation of the CMB. Finally I will discuss how magnetic fields evolve in the post-recombination regime and their impact on structure formation
Elia Battistelli