TALYS is a software package for the simulation of nuclear reactions below 200 MeV. It is
used worldwide for the analysis and prediction of nuclear reactions and is based on state-of …

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 …

Nucleosynthesis in the s process takes place in the He-burning layers of low-mass
asymptotic giant branch (AGB) stars and during the He-and C-burning phases of massive …

The r-process, or the rapid neutron-capture process, of stellar nucleosynthesis is called for to
explain the production of the stable (and some long-lived radioactive) neutron-rich nuclides …

We present the first calculations to follow the evolution of all stable nuclei and their
radioactive progenitors in stellar models computed from the onset of central hydrogen …

Hans Bethe contributed in many ways to our understanding of the supernovae that happen
in massive stars, but, to this day, a first principles model of how the explosion is energized is …

The p-process of stellar nucleosynthesis is aimed at explaining the production of the stable
neutron-deficient nuclides heavier than iron that are observed up to now in the solar system …

A century ago, nuclear physics entered astrophysics, giving birth to a new field of science
referred to as “Nuclear Astrophysics”. With time, it developed at an impressive pace into a …

Context. Nuclear reaction rates of astrophysical applications are traditionally determined on
the basis of Hauser-Feshbach reaction codes. These codes adopt a number of …