There is overwhelmingly experimental evidence indicating that excited nuclear states are
dominated by quasiparticle (qp) excitations, which form many-body configurations with …

The energies and B (E 2) transitions involving the states of the ground-and γ-bands in thirty
transitional and deformed nuclei are calculated using the triaxial projected shell model …

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 …

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

A systematic study of γ γ-bands observed in atomic nuclei is performed using the triaxial
projected shell model (TPSM) approach. The staggering phase between the even and odd …

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 …

The triaxial projected shell model (TPSM) approach is generalized to investigate the
negative parity band structures in even-even systems. In the earlier version of the TPSM …