We use the finite-amplitude method for computing charge-changing Skyrme–quasiparticle
random-phase approximation (QRPA) transition strengths in axially-deformed nuclei …

We present a coupled quasiparticle random phase approximation and Hauser-Feshbach
(QRPA+ HF) model for calculating delayed particle emission. This approach uses …

A new theoretical approach to spin-isospin excitations in open-shell nuclei is presented. The
developed method is based on the relativistic meson-exchange nuclear Lagrangian of …

Background: β-decay rates of neutron-rich nuclei are a crucial ingredient in simulations of
the r-process nucleosynthesis. Up to now global calculations of these rates have been …

β-decay properties of even-and odd-A neutron-rich Ge, Se, Kr, Sr, Ru, and Pd isotopes
involved in the astrophysical rapid neutron capture process are studied within a deformed …

The β-decay half-lives of four semimagic and magic nuclei, Si 34, Ni 68, 78, and Sn 132,
have been investigated using the self-consistent Hartree-Fock (HF) plus subtracted second …

A comparative study of the nuclear Gamow–Teller response (GTR) within conceptually
different state-of-the-art approaches is presented. Three nuclear microscopic models are …

We propose a novel shell-model method to calculate stellar electron-capture (EC) rates of
highly-excited nuclear states. This method is based on the Projected Shell Model that can …

Capture of electrons by nuclei is an important process in stellar environments where excited
nuclear states are thermally populated. However, accurate treatment for excited …

β-delayed neutron emission is one of the key ingredients for astrophysical r-process
nucleosynthesis, and theoretical model predictions have still large uncertainties. In this work …