Speaker
Constança Providencia
(Universidade de Coimbra)
Description
Taking into account experimental data, theoretical calculations and neutron star observations to constrain the equation of state several properties of neutron stars will be discussed, in particular: possible properties of hybrid stars, the influence of hyperonic degrees of freedom on the cooling of neutron stars, the presence of light clusters in the warm equation of state and the effect of the magnetic field on the crust core transition.
Primary author
Constança Providencia
(Universidade de Coimbra)
