Neutron-star matter within the energy-density functional theory and neutron-star structure
Anthea Francesca Fantina, N. Chamel, John Michael Pearson, S. Goriely
Abstract
Anthea Francesca Fantina, N. Chamel, John Michael Pearson, S. Goriely
Abstract
In this lecture, we will present some nucleonic equations of state of neutron-star matter calculated within the nuclear energy-density functional theory using generalized Skyrme functionals developed by the Brussels-Montreal collaboration. These equations of state provide a consistent description of all regions of a neutron star. The global structure of neutron stars predicted by these equations of state will be discussed in connection with recent astrophysical observations.
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In this lecture, we will present some nucleonic equations of state of neutron-star matter calculated within the nuclear energy-density functional theory using generalized Skyrme functionals developed by the Brussels-Montreal collaboration. These equations of state provide a consistent description of all regions of a neutron star. The global structure of neutron stars predicted by these equations of state will be discussed in connection with recent astrophysical observations.
Key concepts: Neutron star, Physics, Equation of state, Neutron, Star (game theory), Dense matter, Nuclear physics, State (computer science)