The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

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 …

The atomic nucleus is a quantum many-body system whose constituent nucleons (protons
and neutrons) are subject to complex nucleon-nucleon interactions that include spin-and …

The astrophysical rapid neutron capture process or 'r process' of nucleosynthesis is believed
to be responsible for the production of approximately half the heavy element abundances …

The rapid neutron capture process (r process) is believed to be responsible for about half of
the production of the elements heavier than iron and contributes to abundances of some …

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 …

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 …

A statistical model for the equation of state and the composition of supernova matter is
presented. It consists of an ensemble of nuclei and interacting nucleons in nuclear statistical …

Background: The mass, or binding energy, is the basis property of the atomic nucleus. It
determines its stability and reaction and decay rates. Quantifying the nuclear binding is …

Nuclear masses are predicted with the Bayesian neural networks by learning the mass
surface of even-even nuclei and the correlation energies to their neighboring nuclei. By …