We propose a projected shell model (PSM) for description of stellar weak-interaction rates
between even-even and odd-odd nuclei with extended configuration space where up to six …

The excited-state structure of atomic nuclei can modify nuclear processes in stellar
environments. In this Letter, we study the influence of nuclear excitations on Urca cooling …

The Wigner rotation matrix (d function), which appears as a part of the angular-momentum-
projection operator, plays a crucial role in modern nuclear-structure models. However, it is a …

Nuclear β spectrum and the corresponding (anti) neutrino spectrum play important roles in
many aspects of nuclear astrophysics, particle physics, nuclear industry, and nuclear data. In …

Chaoticity in nuclei is usually measured by the information entropy through analyzing wave
functions, or by spectral statistics with the spectral rigidity and the nearest neighbor level …

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 …

The finite-temperature linear response theory based on the finite-temperature relativistic
Hartree-Bogoliubov (FT-RHB) model is developed in the charge-exchange channel to study …

We present a Pfaffian formula to calculate matrix elements of three-body operators in
symmetry-restoration beyond-mean-field methods, including the case of multiple …

We propose a theoretical method to calculate the bound-state β-decay half-lives of highly
ionized atoms, which is based on the combination of the Takahashi-Yokoi model and our …