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 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 …

The atomic nucleus is a quantum many-body system whose constituent nucleons (protons
and neutrons) are subject to complex nucleon-nucleon interactions that include spin-and …

A new parametrization PC-PK1 for the nuclear covariant energy density functional with
nonlinear point-coupling interaction is proposed by fitting to observables of 60 selected …

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 …

Symmetry plays a fundamental role in physics. The quasi-degeneracy between single-
particle orbitals (n, l, j= l+ 1/2) and (n− 1, l+ 2, j= l+ 3/2) indicates a hidden symmetry in …

The Possibility of the Secondary Object in GW190814 as a Neutron Star - IOPscience This
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …

The new thorium isotope Th 207 has been produced in the 5 n evaporation channel of the
fusion reaction Ar 36+ Hf 176. It was separated in flight by the gas-filled recoil separator …

Nuclear structure models built from phenomenological mean fields, the effective nucleon–
nucleon interactions (or Lagrangians), and the realistic bare nucleon–nucleon interactions …

The basic concepts and recent developments in the time-dependent density-functional
theory (TDDFT) for describing nuclear dynamics at low energy are presented. The symmetry …