This contribution reviews the present status on the available constraints to the nuclear
equation of state (EoS) around saturation density from nuclear structure calculations on …

Constraints set on key parameters of the nuclear matter equation of state (EoS) by the
values of the tidal deformability, inferred from GW170817, are examined by using a diverse …

The detection of GW170817 in gravitational waves provides unprecedented constraints on
the equation of state (EOS) of the ultradense matter within the cores of neutron stars (NSs) …

The uncertainties in neutron star radii and crust properties due to our limited knowledge of
the equation of state are quantitatively analyzed. We first demonstrate the importance of a …

Background: The microscopic composition and properties of infinite hadronic matter at a
wide range of densities and temperatures have been subjects of intense investigation for …

We study the mass-radius curve of hybrid stars, assuming a single first-order phase
transition between nuclear and quark matter, with a sharp interface between the quark …

The information on the symmetry energy and its density dependence is deduced by
comparing the available data on the electric dipole polarizability α D of Ni 68, Sn 120, and …

The high-density behavior of nuclear matter is analyzed within a relativistic mean field
description with nonlinear meson interactions. To assess the model parameters and their …

Covariant density functional theory is a modern theoretical tool for the description of nuclear
structure phenomena. The current investigation aims at the global assessment of the …

The recent high-resolution measurement of the electric dipole (E 1) polarizability α D in 208
Pb [A. Tamii, Phys. Rev. Lett. 107, 062502 (2011) PRLTAO 0031-9007 …