Séminaire / Seminar GReCO |
| « Numerical models of isolated relativistic stars. » |
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J. Novak |
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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. |
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lundi 30 mai 2016 - 11:00 Salle des séminaires Évry Schatzman Institut d'Astrophysique de Paris |
| Pages web du séminaire / Seminar's webpage |