Behaviour of pf shell under RMF+BCS Description
arXiv:1704.08421 · doi:10.1016/j.cjph.2017.03.022
Abstract
We have employed RMF+BCS (relativistic mean-field plus BCS) approach to study behaviour of pf shell with the help of ground state properties of even-even nuclei. Our present investigations include separation energies , deformations, single particle energies, wavefunction, potential as well etc density distribution. As per recent experiments showing neutron magicity at N = 32 for Ca isotopes, our results with mass dependent pairing indicate a shell closure at N = 32 in Ca isotopes and a more strong shell closure at N = 34 in proton deficient 48Si because of reorganization of neutron pf shell. In a similar manner, proton pf shell structure is more likely to produce shell closure at Z = 34 with a doubly magic character for 84,116Se. We have also included N = 40 isotones and Z = 40 isotopes for our study and predicted 60Ca and 68Ni as doubly magic nuclei out of which 60Ca is found near dripline of Ca and a potential candidate for future studies in the chain of Ca isotopes next to doubly magic 52Ca.
References in corpus (14)
- Collapse of the N=28 shell closure in Si
- Cross-shell excitation in two-proton knockout: Structure of Ca
- Probing the N = 32 shell closure below the magic proton number Z = 20: Mass measurements of the exotic isotopes 52,53K
- New precision mass measurements of neutron-rich calcium and potassium isotopes and three-nucleon forces
- Pairing correlations and resonant states in the relativistic mean field theory
- Magicity of neutron-rich isotopes within relativistic self-consistent approaches
- Proton and neutron skins of light nuclei within the Relativistic Mean Field theory
- A mean field study of single-particle spectra evolution in Z=14 and N=28 chains
- Numerically Fitting The Electron Fermi Energy and The Electron Fraction in A Neutron Star
- Magicity of the Ca and Ca isotopes and tensor contribution within a mean--field approach
- Covariant density functional analysis of shape evolution in isotones
- Neutron and spin--orbit splittings in Ca, S, and Si isotones: tensor--induced and pure spin--orbit effects
- Shell structure from nuclear observables
- Determination of hadron-quark phase transition line from lattice QCD and two-solar-mass neutron star observations