Density distributions of superheavy nuclei
arXiv:nucl-th/0507052 · doi:10.1103/PhysRevC.71.034302
Abstract
We employed the Skyrme-Hartree-Fock model to investigate the density distributions and their dependence on nuclear shapes and isospins in the superheavy mass region. Different Skyrme forces were used for the calculations with a special comparison to the experimental data in Pb. The ground-state deformations, nuclear radii, neutron skin thicknesses and -decay energies were also calculated. Density distributions were discussed with the calculations of single-particle wavefunctions and shell fillings. Calculations show that deformations have considerable effects on the density distributions, with a detailed discussion on the 120 nucleus. Earlier predictions of remarkably low central density are not supported when deformation is allowed for.
7 pages, 10 figures
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- Central depression in nucleonic densities: Trend analysis in nuclear density-functional-theory approach
- Time-dependent HF approach to SHE dynamics
- Isotopic trends of quasifission and fusion-fission in the reactions Ca+Pu
- Structure of superheavy nuclei
- Bubble nuclei: single-particle versus Coulomb interaction effects
- Impacts of the tensor couplings of and mesons and Coulomb exchange terms on super-heavy nuclei and their relation to symmetry energy
- Quantum and Coulomb repulsion effects on the bubble structures in Hg