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 …

Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …

Background: The microscopic composition and properties of infinite hadronic matter at a
wide range of densities and temperatures have been subjects of intense investigation for …

We propose the existence of a lower bound on the energy of pure neutron matter (PNM) on
the basis of unitary-gas considerations. We discuss its justification from experimental studies …

The uncertainties in neutron star radii and crust properties due to our limited knowledge of
the equation of state are quantitatively analyzed. We first demonstrate the importance of a …

We infer the mass distribution of neutron stars in binary systems using a flexible Gaussian
mixture model and use Bayesian model selection to explore evidence for multimodality and …

In this review we first outline the basics of transport theory and its recent generalization to off-
shell transport. We then present in some detail the main ingredients of any transport method …

We investigate nuclear matter at a finite temperature and density, including the formation of
light clusters up to the α particle (1⩽ A⩽ 4). The novel feature of this work is to include the …

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 …

We introduce a parametrized high-density equation of state (EOS) in order to systematize
the study of constraints placed by astrophysical observations on the nature of neutron-star …