Résumé / Abstract Seminaire_GReCO

"Numerical models of isolated relativistic stars."

J. Novak

Realistic global neutron star models require numerical approach. In this talk, I shall briefly motivate and recall the general-relativistic framework for the description of rotating compact stars and show how global observable quantities can be computed unambiguously. Then, I will present some recent results on the building of more detailed physical models, including realistic microphysics, following two directions. First, I shall describe the inclusion of magnetic field and its effects on both, global equilibrium and equation of state, then I will discuss superfluid (two-fluid) models in an attempt to model glitch phenomena.

lundi 30 mai 2016 - 11:00
Salle des séminaires Évry Schatzman,
Institut d'Astrophysique de Paris

Page web du séminaire / Seminar's webpage