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 …

Many of the currently available equations of state for core-collapse supernova simulations
give large neutron star radii and do not provide large enough neutron star masses, both of …

The nuclear symmetry energy characterizes the variation of the binding energy as the
neutron to proton ratio of a nuclear system is varied. This is one of the most important …

Transport simulations are very valuable for extracting physics information from heavy-ion-
collision experiments. With the emergence of many different transport codes in recent years …

We develop new hyperon equation of state (EoS) tables for core-collapse supernova
simulations and neutron stars. These EoS tables are based on a density-dependent …

We develop a kinetic approach to the production of light nuclei up to mass number A⩽ 4 in
intermediate-energy heavy-ion collisions by including them as dynamic degrees of freedom …

A review is given on the studies of formation of light clusters and heavier fragments in heavy-
ion collisions at incident energies from several tens of MeV/nucleon to several hundred …

We compute from chiral two-and three-nucleon interactions the energy per particle of
symmetric nuclear matter and pure neutron matter at third-order in perturbation theory …

It is studied how the α cluster degrees of freedom, such as α clustering configurations close
to the α decay threshold in C 12 and O 16, including the linear chain, triangle, square, kite …