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 …

Neutrino–nuclear responses associated with astro-neutrinos, single beta decays and double
beta decays are crucial in studies of neutrino properties of interest for astro-particle physics …

Bayesian neural network (BNN) approach is employed to improve the nuclear mass
predictions of various models. It is found that the noise error in the likelihood function plays …

Background: r-process nucleosynthesis models rely, by necessity, on nuclear structure
models for input. Particularly important are β-decay half-lives of neutron-rich nuclei. At …

This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star
merger GW170817 was observed in extraordinary detail with gravitational waves and …

Nuclear structure models built from phenomenological mean fields, the effective nucleon–
nucleon interactions (or Lagrangians), and the realistic bare nucleon–nucleon interactions …

The basic concepts and recent developments in the time-dependent density-functional
theory (TDDFT) for describing nuclear dynamics at low energy are presented. The symmetry …

Nuclear β decay is a key process to understand the origin of heavy elements in the universe,
while the accuracy is far from satisfactory for the predictions of β-decay half-lives by nuclear …

We have performed r-process calculations for matter ejected dynamically in neutron star
mergers based on a complete set of trajectories from a three-dimensional relativistic …

Nuclear weak decays provide important probes to fundamental symmetries in nature. A
precise description of these processes in atomic nuclei requires comprehensive knowledge …