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 …

We review the physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …

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

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

Collisions involving Sn 112 and Sn 124 nuclei have been simulated with the improved
quantum molecular dynamics transport model. The results of the calculations reproduce …

Model Comparison from LIGO–Virgo Data on GW170817’s Binary Components and
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …

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 …

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 …

We propose the existence of a lower bound on the energy of pure neutron matter (PNM) on
the basis of unitary-gas considerations. We discuss its justification from experimental studies …

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 …