We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

We tabulate the atomic mass excesses and binding energies, ground-state shell-plus-
pairing corrections, ground-state microscopic corrections, and nuclear ground-state …

A review is made of constraints on the nuclear symmetry energy parameters arising from
nuclear binding energy measurements, theoretical chiral effective field predictions of …

Recent developments in the theory of pure neutron matter and experiments concerning the
symmetry energy of nuclear matter, coupled with recent measurements of high-mass …

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 …

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 …

The symmetry energy contribution to the nuclear equation of state impacts various
phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its …

This paper presents a detailed assessment of the ability of the 240 Skyrme interaction
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …

The nuclear symmetry energy characterizes the variation of the binding energy as the
neutron to proton ratio of a nuclear system is varied. This is one of the most important …