Orateur
Constança Providência
(University of Coimbra)
Description
Semiclassical methods in nuclear physics are a very good tool to study the behavior and composition of neutron stars. Using the Vlasov equation, the neutron star crust-core transition will be discussed, also in the presence of a strong magnetic field as expected inside magnetars. The description of the inner crust within a Thomas Fermi approach will be presented.
Auteur principal
Constança Providência
(University of Coimbra)
