Metamodeling for the nucleonic equation of state (EOS), inspired from a Taylor expansion
around the saturation density of symmetric nuclear matter, is proposed and parameterized in …

We construct the equation of state (EOS) of nuclear matter using the relativistic mean field
(RMF) theory in the wide density, temperature range with various proton fractions for the use …

Background. We investigate possible correlations between neutron star observables and
properties of atomic nuclei. In particular, we explore how the tidal deformability of a 1.4 solar …

The constituents of cold dense matter are still far from being understood. However, neutron
star observations such as the recently observed pulsar PSR J1614-2230 with a mass of …

We construct the equation of state (EOS) of nuclear matter at finite temperature and density
with various proton fractions within the relativistic mean field (RMF) theory for use in …

The standard variational derivation of stellar-matter structure in the Wigner-Seitz
approximation is generalized to the finite-temperature situation where a wide distribution of …

We perform a systematic analysis of the density dependence of nuclear symmetry energy
within the microscopic Brueckner-Hartree-Fock (BHF) approach using the realistic Argonne …

We study the evolution of a supernova core from the beginning of the gravitational collapse
of a 15 M☉ star up to 1 s after core bounce. We present results of spherically symmetric …

The possibility to draw links between the isospin properties of nuclei and the structure of
compact stars is a stimulating perspective. In order to pursue this objective on a sound basis …

We study black hole formation and the neutrino signal from the gravitational collapse of a
nonrotating massive star of 40 M☉. Adopting two different sets of realistic equations of state …