We present a review of a broad selection of nuclear matter equations of state (EOSs)
applicable in core-collapse supernova studies. The large variety of nuclear matter …

Light clusters (mass number A≤ 4) in nuclear matter at subsaturation densities are
described using a quantum statistical approach to calculate the quasiparticle properties and …

The pasta phase in core-collapse supernova matter (finite temperatures and fixed proton
fractions) is studied within relativistic mean-field models. Three different calculations are …

Cluster formation is a fundamental aspect of the equation of state (EOS) of warm and dense
nuclear matter such as can be found in supernovae (SNe). Similar matter can be studied in …

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

The formation of clusters at sub-saturation densities, as a result of many-body correlations,
constitutes an essential feature for a reliable modelization of the nuclear matter equation of …

The pasta phases are calculated for warm stellar matter in a framework of relativistic mean-
field models, including the possibility of light cluster formation. Results from three different …

The spinodal instabilities in hot asymmetric nuclear matter and some important critical
parameters derived thereof are studied by using six different families of relativistic mean …