5 papers
Thermal evolution of neo-neutron stars. II. Temperature-dependent crusts
Sagnik Chatterjee, Mikhail V. Beznogov, Dany Page +1
The neo-neutron star phase is an intermediate stage in the evolution from a hot lepton-rich compact object, which is formed in the aftermath of a core-collapse supernova or an accr…
Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions: A generalization
Mikhail V. Beznogov, Adriana R. Raduta
The nonrelativistic theory of nuclear matter (NM) based on Brussels-Skyrme interactions is employed to develop models for dense and neutron-rich matter within a Bayesian framework.…
On the Inner Crusts of Neo-Neutron Stars: exotic light nuclei, diffusional and thermodynamical stability
Mikhail V. Beznogov, Adriana R. Raduta
Based on an extended nuclear statistical equilibrium model, we investigate the properties of non-accreted crusts of young and warm neo-neutron stars, i.e., of finite-temperature in…
New ab initio constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: II. Thermal response in the suprasaturation density domain
Adriana R. Raduta, Mikhail V. Beznogov
Numerical simulations of core-collapse supernovae, mergers of binary neutron stars and formation of stellar black holes, which employed standard Skyrme interactions, established cl…
New {\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain
Adriana R. Raduta, Mikhail V. Beznogov
In numerical simulations of core-collapse supernova and binary neutron stars mergers, information about the energetics and composition of matter is implemented via external tables…