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 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 …

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 …

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 …

This contribution reviews the present status on the available constraints to the nuclear
equation of state (EoS) around saturation density from nuclear structure calculations on …

The ultimate goal of studying isospin physics via heavy-ion reactions with neutron-rich,
stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear …

Relativistic energy density functionals (EDF) have become a standard tool for nuclear
structure calculations, providing a complete and accurate, global description of nuclear …

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 …

We study a particular class of relativistic nuclear energy density functionals in which only
nucleon degrees of freedom are explicitly used in the construction of effective interaction …

Various kinds of isovector nucleon effective masses are used in the literature to characterize
the momentum/energy dependence of the nucleon symmetry potential or self-energy due to …