The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …

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 …

Transport models are the main method to obtain physics information on the nuclear equation
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …

The density dependence of nuclear symmetry energy is among the most uncertain parts of
the Equation of State (EOS) of dense neutron-rich nuclear matter. It is currently poorly known …

Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …

The atomic nucleus is one of the densest and most complex quantum-mechanical systems
in nature. Nuclei account for nearly all the mass of the visible Universe. The properties of …

We study the impact of finite-temperature effects in numerical-relativity simulations of binary
neutron star mergers with microphysical equations of state and neutrino transport in which …

We use Stergioulas's RNS code for investigating fast pulsars with equations of state (EOSs)
on the causality surface (where the speed of sound is equal to that of light) of the high …

While mean-field approximations, such as the nuclear shell model, provide a good
description of many bulk nuclear properties, they fail to capture the important effects of …

Within the parameter space of the equation of state (EOS) of dense neutron-rich matter
limited by existing constraints mainly from terrestrial nuclear experiments, we investigate …