Speaker
Dr
Micaela Oertel
(Meudon Observatory)
Description
In this talk I will present a temperature dependent equation of
state (EoS) including the entire baryon octet, being compatible with
the main constraints from nuclear physics and, in particular, with a
maximum mass for cold $\beta$-equilibrated neutron stars of
$2M_\odot$ in agreement with recent observations. As an application,
numerical stationary models for rapidly (rigidly) rotating hot
neutron stars have been computed. I will discuss their maximum
masses and the universality of $I$-$Q$-relations at nonzero
temperature for fast rotating models.
| Type of contribution | Invited talk |
|---|
Primary author
Dr
Micaela Oertel
(Meudon Observatory)
