Isospin-symmetry breaking is responsible for the energy difference of excited states in mirror
nuclei. It also influences the coefficient of the isobaric multiplet mass equation. In the present …

Abstract Since Mayer and Jensen employed the single-particle shell model to interpret the
magic numbers, various microscopic nuclear models have been developed to study the …

The paper reviews the recent progress in the description of isospin-symmetry breaking
within the nuclear shell model and applications to actual problems related to the structure …

β decay of proton-rich nuclei plays an important role in exploring isospin mixing. The β
decay of P 26 at the proton drip line is studied using double-sided silicon strip detectors …

With both three-nucleon force and continuum coupling included, we have developed a self-
consistent ab initio Gamow shell model within the Gamow Hartree-Fock (GHF) basis …

Neutronic performance is investigated for a potential accident tolerant fuel (ATF), which
consists of U3Si2 fuel and FeCrAl cladding. In comparison with current UO2‐Zr system …

The ground-state mass excess of the Tz=− 2 drip-line nucleus 22Al is measured for the first
time to be 18103 (10) keV using the newly-developed Bρ-defined isochronous mass …

Background: β-decay spectroscopy provides valuable nuclear physics input for accurate
modeling of nova and x-ray burst observables and a stringent test for shell-model theories …

The β decay of P 26 was used to populate the astrophysically important E x= 5929.4 (8) keV,
J π= 3+ state of Si 26. Both β-delayed protons at 418 (8) keV and γ rays at 1742 (2) keV …

The decay of the lightest nucleus with T z=− 3, 22 Si, was studied by a silicon array. A
charged-particle group at 5600 (70) keV in the decay-energy spectrum was identified …