Towards understanding astrophysical effects of nuclear symmetry energy
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
Hidden pseudospin and spin symmetries and their origins in atomic nuclei
Symmetry plays a fundamental role in physics. The quasi-degeneracy between single-
particle orbitals (n, l, j= l+ 1/2) and (n− 1, l+ 2, j= l+ 3/2) indicates a hidden symmetry in …
particle orbitals (n, l, j= l+ 1/2) and (n− 1, l+ 2, j= l+ 3/2) indicates a hidden symmetry in …
Towards an ab initio covariant density functional theory for nuclear structure
Nuclear structure models built from phenomenological mean fields, the effective nucleon–
nucleon interactions (or Lagrangians), and the realistic bare nucleon–nucleon interactions …
nucleon interactions (or Lagrangians), and the realistic bare nucleon–nucleon interactions …
Halos in medium-heavy and heavy nuclei with covariant density functional theory in continuum
Covariant density functional theory with a few parameters has been widely used to describe
the ground-and excited-state properties for nuclei all over the nuclear chart. In order to …
the ground-and excited-state properties for nuclei all over the nuclear chart. In order to …
Isospin corrections for superallowed Fermi decay in self-consistent relativistic random-phase approximation approaches
Self-consistent random phase approximation (RPA) approaches in the relativistic framework
are applied to calculate the isospin symmetry-breaking corrections δ c for the 0+→ 0+ …
are applied to calculate the isospin symmetry-breaking corrections δ c for the 0+→ 0+ …
Relativistic Hartree-Fock-Bogoliubov theory with density dependent meson-nucleon couplings
Relativistic Hartree-Fock-Bogoliubov (RHFB) theory with density-dependent meson-nucleon
couplings is presented. The integrodifferential RHFB equations are solved by expanding the …
couplings is presented. The integrodifferential RHFB equations are solved by expanding the …
Dense matter equation of state of a massive neutron star with antikaon condensation
Recent measurements of neutron star mass from several candidates (PSR J 1614-2230,
PSR J 0348+ 0432, MSP J 0740+ 6620) set the lower bound on the maximum possible …
PSR J 0348+ 0432, MSP J 0740+ 6620) set the lower bound on the maximum possible …
Relativistic Hartree-Fock-Bogoliubov model for axially deformed nuclei
J Geng, WH Long - Physical Review C, 2022 - APS
Background: At the forefront of nuclear science, unstable nuclei are of special significance,
in which the deformation and pairing correlations play an essential role in determining the …
in which the deformation and pairing correlations play an essential role in determining the …
Quantitative analysis of tensor effects in the relativistic Hartree-Fock theory
Tensor force is identified in each meson-nucleon coupling in the relativistic Hartree-Fock
theory. It is found that all the meson-nucleon couplings, except the σ-scalar one, give rise to …
theory. It is found that all the meson-nucleon couplings, except the σ-scalar one, give rise to …
effects in density-dependent relativistic Hartree-Fock theory and neutron stars
The density-dependent relativistic Hartree-Fock (DDRHF) theory is extended to include Δ
isobars for the study of dense nuclear matter and neutron stars. To this end, we solve the …
isobars for the study of dense nuclear matter and neutron stars. To this end, we solve the …