Published November 2011 | Version v1
Journal article

Collective structural evolution in neutron-rich Yb, Hf, W, Os, and Pt isotopes

  • 1. Department of Physics, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)
  • 2. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321 (United States)
  • 3. Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)
  • 4. Instituto de Estructura de la Materia, IEM-CSIC, Serrano 123, E-28006 Madrid (Spain)
  • 5. Departamento de Fisica Teorica, Universidad Autonoma de Madrid, E-28049 Madrid (Spain)

Description

An interacting-boson-model Hamiltonian determined from Hartree-Fock-Bogoliubov calculations with the microscopic Gogny energy density functional D1M is applied to the spectroscopic analysis of neutron-rich Yb, Hf, W, Os, and Pt isotopes with mass A∼180-200. Excitation energies and transition rates for the relevant low-lying quadrupole collective states are calculated by this method. Transitions from prolate to oblate ground-state shapes are analyzed as a function of neutron number N in a given isotopic chain by calculating excitation energies, B(E2) ratios, and correlation energies in the ground state. It is shown that such transitions tend to occur more rapidly for the isotopes with lower proton number Z when departing from the proton shell closure Z=82. The triaxial degrees of freedom turn out to play an important role in describing the considered mass region. Predicted low-lying spectra for the neutron-rich exotic Hf and Yb isotopes are presented. The approximations used in the model and the possibilities to refine its predictive power are addressed.

Additional details

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
84
Journal Issue
5
Journal Page Range
p. 054316-054316.11
ISSN
0556-2813
CODEN
PRVCAN

Optional Information

Notes
(c) 2011 American Institute of Physics