Yrast γ-ray spectroscopy of the neutron rich isotopes Co61,63

P. H. Regan, J. W. Arrison, U. J. Hüttmeier, and D. P. Balamuth
Phys. Rev. C 54, 1084 – Published 1 September 1996
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Abstract

The neutron rich nuclei Co61,63 have been studied using the reactions O16(48Ca,p2n)61Co and O18(48Ca,p2n)63Co at a bombarding energy of 110 MeV. Discrete γ rays from the channels of interest were investigated using prescaled γ singles, charged-particle–γ, neutron–charged-particle–γ, and charged-particle–γ–γ coincidence techniques. Decay schemes, with level spins deduced from two-point angular distribution data, are presented together with some approximate information on apparent state lifetimes. The experimental results are compared with previous light ion data for these systems and with theoretical shell model predictions. These data represent the first study of medium to high spin states in these nuclei. © 1996 The American Physical Society.

  • Received 29 April 1996

DOI:https://doi.org/10.1103/PhysRevC.54.1084

©1996 American Physical Society

Authors & Affiliations

P. H. Regan, J. W. Arrison, U. J. Hüttmeier, and D. P. Balamuth

  • Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104
  • Department of Physics, University of Surrey, Guildford, GU2 5XH, United Kingdom

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Vol. 54, Iss. 3 — September 1996

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