Neutron stars provide a window into the properties of dense nuclear matter. Several recent
observational and theoretical developments provide powerful constraints on their structure …

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 …

Laboratory experiments sensitive to the equation of state of neutron rich matter in the vicinity
of nuclear saturation density provide the first rung in a “density ladder” that connects …

Heavy atomic nuclei have an excess of neutrons over protons, which leads to the formation
of a neutron skin whose thickness is sensitive to details of the nuclear force. This links …

We present the results of an improved Monte Carlo Glauber (MCG) model of relevance for
collisions involving nuclei at center-of-mass energies of the BNL Relativistic Heavy Ion …

A review is made of constraints on the nuclear symmetry energy parameters arising from
nuclear binding energy measurements, theoretical chiral effective field predictions of …

A bstract We present a new model for building up complete exclusive hadronic final states in
high energy nucleus collisions. It is a direct extrapolation of high energy pp collisions (as …

What is the size of the atomic nucleus? This deceivably simple question is difficult to answer.
Although the electric charge distributions in atomic nuclei were measured accurately already …

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 …

We review the theoretical and experimental progress in the Glauber model of multiple
nucleon and/or parton scatterings after the last 10–15 years of operation with proton and …