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 …

Metamodeling for the nucleonic equation of state (EOS), inspired from a Taylor expansion
around the saturation density of symmetric nuclear matter, is proposed and parameterized in …

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 …

Our family of three Hartree-Fock-Bogoliubov (HFB) mass models, labeled BSk19, BSk20,
and BSk21, is here extended by (a) refitting to the 2012 Atomic Mass Evaluation (AME), and …

Traditional photonuclear reactions primarily excite giant dipole resonances, making the
measurement of isovector giant resonances with higher multipolarities a great challenge. In …

The information on the symmetry energy and its density dependence is deduced by
comparing the available data on the electric dipole polarizability α D of Ni 68, Sn 120, and …

Using excitation energies to isobaric analog states (IAS) and charge invariance, we extract
nuclear symmetry coefficients, representing a mass formula, on a nucleus-by-nucleus basis …

This review aims at providing an extensive discussion of modern constraints relevant for
dense and hot strongly interacting matter. It includes theoretical first-principle results from …

A feed-forward neural network model is trained to calculate the nuclear charge radii. The
model is trained with the input data set of proton and neutron number Z, N, the electric …