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 …

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 …

Abstract According to the Hugenholtz–Van Hove theorem, nuclear symmetry energy E sym
(ρ) and its slope L (ρ) at an arbitrary density ρ are determined by the nucleon isovector …

The need to reconcile our understanding of the behavior of hadronic matter across a wide
range of densities, especially at the time when data from multimessenger observations and …

We show that the neutron skin thickness Δ rnp of heavy nuclei is uniquely fixed by the
symmetry energy density slope L (ρ) at a subsaturation cross density ρ c≈ 0.11 fm− 3 rather …

We study the electric dipole polarizability α D in 208 Pb based on the predictions of a large
and representative set of relativistic and nonrelativistic nuclear mean-field models. We adopt …

Recent improvements in the experimental determination of properties of the isovector giant
quadrupole resonance (IVGQR), as demonstrated in the A= 208 mass region, may be …

Using the recent model-independent determination of the charge-weak form factor
difference Δ F CW in Ca 48 and Pb 208 by the CREX and PREX-2 collaborations together …

The density dependence of the symmetry energy around saturation density, characterized
by the slope parameter L, is studied using information provided by the neutron skin …

Relations between the nuclear symmetry energy coefficient and its density derivatives are
derived. The relations hold for a class of interactions with quadratic momentum dependence …