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 …

Context. Proto-neutron stars are born hot, with temperatures exceeding a few times 10 10 K.
In these conditions, the crust of the proto-neutron star is expected to be made of a Coulomb …

Context. The crust of a neutron star is known to melt at a temperature that increases with
increasing matter density, up to about 10 10 K. At such high temperatures and beyond, the …

Nuclear pasta topology is an essential ingredient to determine transport properties in the
inner crust of neutron stars. We perform semiclassical molecular dynamics simulations of …

In-medium modifications of light cluster properties in warm stellar matter are studied within
the relativistic mean-field approximation. In-medium effects are included by introducing an …

Light and heavy clusters are calculated for asymmetric warm nuclear matter in a relativistic
mean-field approach. In-medium effects, introduced via a universal cluster-meson coupling …

We investigate the localization and clustering features in Ne 20 (N= Z) and neutron-rich Ne
32 nuclei at zero and finite temperatures. The finite temperature Hartree-Bogoliubov theory …

We study the composition of nuclear matter at sub-saturation densities, non-zero
temperatures, and isospin asymmetry, under the conditions characteristic of binary neutron …

Being born hot from core-collapse supernova, the crust of the proto-neutron star is expected
to be made of a Coulomb liquid and composed of an ensemble of different nuclear species …

The rapidity distributions of hydrogen isotopes emitted from central collisions of neutron-rich
132 Sn+ 124 Sn and neutron-deficient 108 Sn+ 112 Sn systems at 270 MeV/nucleon were …