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 …

One of the most intriguing questions about neutron stars concerns their maximum mass. The
answer is intimately related to the properties of matter at densities far beyond that found in …

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 …

We present the equation of state of infinite neutron matter as obtained from highly realistic
Hamiltonians that include nucleon-nucleon and three-nucleon coordinate-space potentials …

Background: The equation of state (EoS) of nucleonic matter is central for the understanding
of bulk nuclear properties, the physics of neutron star crusts, and the energy release in …

We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the
core based on modern microscopic calculations using the Argonne v 18 potential plus three …

We report benchmark calculations of the energy per particle of pure neutron matter as a
function of the baryon density using three independent many-body methods: Brueckner …

We present calculations for symmetric nuclear matter using chiral nuclear interactions within
the self-consistent Green's functions approach in the ladder approximation. Three-body …

We discuss the “constant speed of sound”(CSS) parametrization of the equation of state of
high-density matter and its application to the field correlator method (FCM) model of quark …

The effects of the ϕ meson on the properties of hyperon stars are studied systematically in
the framework of the density-dependent relativistic mean field (DDRMF) model. The ϕ …