We provide convenient parametrizations of the high-density nuclear equation of state
obtained within the Brueckner-Hartree-Fock approach using different modern nucleon …

We calculate the nucleonic equation of state within the Brueckner-Bethe-Goldstone
formalism using the Argonne υ 18 two-body interaction and a three-body interaction. We …

The energies of symmetric nuclear matter and neutron matter are evaluated in the lowest-
order Brueckner theory using a chiral effective field theory potential including effects of a …

We investigate properties of nuclear matter and examine possible correlations with neutron
star observables for a set of microscopic nuclear equations of state derived within the …

An extremely simple form for the energy density of a nuclear many-body system derived from
the two-body nucleon-nucleon interaction is used to determine the ground state …

We calculate the equation of state of neutron matter with realistic two-and three-nucleon
interactions using quantum Monte Carlo techniques and illustrate that the short-range three …

An accurately calibrated relativistic parametrization is introduced to compute the ground
state properties of finite nuclei, their linear response, and the structure of neutron stars …

We review the calculation of the equation of state of pure neutron matter using quantum
Monte Carlo (QMC) methods. QMC algorithms permit the study of many-body nuclear …

Abstract Properties of dense nucleon matter and the structure of neutron stars are studied
using variational chain summation methods and the new Argonne v 18 two-nucleon …

Using a phenomenological form of the equation of state of neutron matter near the saturation
density which has been previously demonstrated to be a good characterization of quantum …