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Thermal behavior as indicator for hyperons in binary neutron star merger remnants
Sebastian Blacker, Hristijan Kochankovski, Andreas Bauswein +2
We provide the first comprehensive study of hyperons in neutron star mergers and quantify their specific impact. We discuss the thermal behavior of hyperonic equations of state~(Eo…
Equation of state for hot hyperonic neutron star matter
Hristijan Kochankovski, Angels Ramos, Laura Tolos
The FSU2H equation-of-state model, originally developed to describe cold neutron star matter with hyperonic cores, is extended to finite temperature. Results are presented for a wi…
Interplay between Particles and Hyperons in Neutron Stars
Patricia Ribes, Angels Ramos, Laura Tolos +2
We analyze the effects of including isobars in an equation of state (EoS) for cold, -stable neutron star matter, employing relativistic nuclear mean field theory. The…
The Equation of State and Cooling of Hyperonic Neutron Stars
Laura Tolos, Mario Centelles, Angels Ramos +2
We present two recent parametrizations of the equation of state (FSU2R and FSU2H models) that reproduce the properties of nuclear matter and finite nuclei, fulfill constraints on h…
Cooling of Small and Massive Hyperonic Stars
Rodrigo Negreiros, Laura Tolos, Mario Centelles +2
We perform cooling simulations for isolated neutron stars using recently developed equations of state for their core. The equations of state are obtained from new parametrizations…
The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
Laura Tolos, Mario Centelles, Angels Ramos
We reexamine the equation of state for the nucleonic and hyperonic inner core of neutron stars that satisfies the 2 observations as well as the recent determinations of…