Speaker
Massimo Mannarelli
Description
We discuss some properties of superfluids that could be relevant for the evolution of compact stars.
Superfluids emerge in many different systems and can be produced and accurately studied in laboratory.
We will discuss how some of the results recently obtained in laboratory could be employed to better understand the interior of compact stars.
Of particular interest are inhomogeneous superfluid phases, which could emerge within the inner crust of neutron stars and could be emulated employing dipolar ultracold atoms.
