High-spin structure of neutron-rich Se, As, Ge, and Ga isotopes

N. Yoshinaga, K. Higashiyama, and P. H. Regan
Phys. Rev. C 78, 044320 – Published 23 October 2008

Abstract

Full-fledged shell-model calculations have been performed for neutron-rich Se, As, Ge, and Ga isotopes using a valence space made up from nucleons occupying the g9/2,p1/2,p3/2, and f5/2 orbitals. The calculated energies and electromagnetic transitions are compared with the experimental data which is available on these nuclei. Pair-truncated shell model calculations have also been carried out to investigate the structure of the high-spin states, with particular focus on the effect of the alignment of neutrons in the g9/2 orbital.

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  • Received 17 June 2008

DOI:https://doi.org/10.1103/PhysRevC.78.044320

©2008 American Physical Society

Authors & Affiliations

N. Yoshinaga1,*, K. Higashiyama2,†, and P. H. Regan3,‡

  • 1Department of Physics, Saitama University, Saitama City 338-8570, Japan
  • 2Department of Physics, Chiba Institute of Technology, Narashino, Chiba 275-0023, Japan
  • 3Department of Physics, University of Surrey, Guildford GU2 7XH, United Kingdom

  • *yoshinaga@phy.saitama-u.ac.jp
  • koji.higashiyama@it-chiba.ac.jp
  • p.regan@surrey.ac.uk

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Issue

Vol. 78, Iss. 4 — October 2008

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