Large-scale shell-model calculations for unnatural-parity high-spin states in neutron-rich Cr and Fe isotopes
arXiv:1411.3886 · doi:10.1103/PhysRevC.91.024320
Abstract
We investigate unnatural-parity high-spin states in neutron-rich Cr and Fe isotopes using large-scale shell-model calculations. These shell-model calculations are carried out within the model space of -shell + + orbits with the truncation allowing excitation of a neutron. The effective Hamiltonian consists of GXPF1Br for -shell orbits and with a modification for the other parts. The present shell-model calculations can describe and predict the energy levels of both natural- and unnatural-parity states up to the high-spin states in Cr and Fe isotopes with . The total energy surfaces present the prolate deformations on the whole and indicate that the excitation of one neutron into the orbit plays the role of enhancing the prolate deformation. For the positive(unnatural)-parity states in odd-mass Cr and Fe isotopes, their energy levels and prolate deformations indicate the decoupling limit of the particle-plus-rotor model. The sharp drop of the levels in going from to in odd-mass Cr and Fe isotopes is explained by the Fermi surface approaching the orbit.
References in corpus (16)
- The Shell Model as Unified View of Nuclear Structure
- Magic numbers in exotic nuclei and spin-isospin properties of {\it NN} interaction
- Novel features of nuclear forces and shell evolution in exotic nuclei
- New effective interaction for -shell nuclei and its implications for the stability of the ==28 closed core
- Shape transitions in exotic Si and S isotopes and tensor-force-driven Jahn-Teller effect
- Novel shape evolution in exotic Ni isotopes and configuration-dependent shell structure
- Spherical Shell Model description of rotational motion
- Cross-shell excitation in two-proton knockout: Structure of Ca
- Observation of isotonic symmetry for enhanced quadrupole collectivity in neutron-rich 62,64,66Fe isotopes at N=40
- Light Nuclei near Neutron and Proton Drip Lines in the Relativistic Mean-Field Theory
- Shell model study of single-particle and collective structure in neutron-rich Cr isotopes
- An Update of B(E2) Evaluation for 0+1 -> 2+1 Transitions in Even-Even Nuclei near N~Z~28
- Nuclear Structure Towards N=40 60Ca: In-beam gamma-ray Spectroscopy of 58,60Ti
- Variational procedure for nuclear shell-model calculations and energy-variance extrapolation
- Magnetic Moment of the Fragmentation Aligned 61Fe(9/2)+ Isomer
- Deformation around neutron-rich Cr isotopes in axially symmetric Skyrme-Hatree-Fock-Bogoliubov method
Cited by in corpus (17)
- Isomerism in the "south-east" of Sn and a predicted neutron-decaying isomer in Pd
- Time-of-flight mass measurements of neutron-rich chromium isotopes up to N = 40 and implications for the accreted neutron star crust
- Shell-model-like approach based on cranking covariant density functional theory: bandcrossing and shape evolution in Fe
- Double-step truncation procedure for large-scale shell-model calculations
- Masses of ground and isomeric states of In and configuration-dependent shell evolution in odd- indium isotopes
- Occupation numbers of spherical orbits in self-consistent beyond-mean-field methods
- The impact of the off-diagonal cross-shell interaction on C
- decay study of the Mn - Fe - Co - Ni chain
- Search for -cluster states in even-even Cr isotopes
- Shell model results for Ca isotopes in the , and model spaces
- Structure of Ca from the decay of K in the framework of nuclear shell model
- Nuclear Structure Properties of even-even Chromium Isotopes and the E ect of Deformation on Calculated Electron Capture Cross Sections
- Fe(,)Fe and the evolution of single neutron energies in the isotones
- Coexistence of single particle and collective excitation in Ni
- Systematic shell-model study of Cd isotopes and isomers in neutron-rich In isotopes
- Ab initio study of island of inversion in odd- nuclei: Structure of Mg
- Level structure of light neutron-rich La isotopes beyond the N=82 shell closure