In RMF with NL3*, small components of Dirac spinors for neutrons near the Fermi level contribute to the proton potential and help form the kink in Sn charge radii at N=82, with j=l-1/2 states more effective than j=l+1/2, but the effect alone does not fully explain the observed magnitude.
Ring, Prog
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
nucl-th 3years
2026 3representative citing papers
Using microscopically computed inputs from FT-CDFT with PC-PK1, the dinuclear system model reproduces known fusion data and predicts maximum cross sections of 48.20 fb, 12.33 fb, 5.25 fb, and 0.47 fb for four reactions targeting element 120.
Relativistic mean-field calculations with asymmetric finite differences find that neutron-star inner-crust binding energies decrease with larger symmetry-energy slope L and larger nucleon effective mass, while quantum shell effects produce oscillatory densities and alter neutron properties.
citing papers explorer
-
Charge radii of Sn isotopes in the relativistic mean field approximation
In RMF with NL3*, small components of Dirac spinors for neutrons near the Fermi level contribute to the proton potential and help form the kink in Sn charge radii at N=82, with j=l-1/2 states more effective than j=l+1/2, but the effect alone does not fully explain the observed magnitude.
-
Synthesis mechanism of superheavy element 120: a dinuclear system model approach with microscopic inputs
Using microscopically computed inputs from FT-CDFT with PC-PK1, the dinuclear system model reproduces known fusion data and predicts maximum cross sections of 48.20 fb, 12.33 fb, 5.25 fb, and 0.47 fb for four reactions targeting element 120.
-
Relativistic mean-field study of the neutron star inner crust using the asymmetric finite difference method
Relativistic mean-field calculations with asymmetric finite differences find that neutron-star inner-crust binding energies decrease with larger symmetry-energy slope L and larger nucleon effective mass, while quantum shell effects produce oscillatory densities and alter neutron properties.