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New low-energy 0+ state and shape coexistence in Ni70

C. J. Prokop, B. P. Crider, S. N. Liddick, A. D. Ayangeakaa, M. P. Carpenter, J. J. Carroll, J. Chen, C. J. Chiara, H. M. David, A. C. Dombos, S. Go, J. Harker, R. V. F. Janssens, N. Larson, T. Lauritsen, R. Lewis, S. J. Quinn, F. Recchia, D. Seweryniak, A. Spyrou, S. Suchyta, W. B. Walters, and S. Zhu
Phys. Rev. C 92, 061302(R) – Published 21 December 2015

Abstract

In recent models, the neutron-rich Ni isotopes around N=40 are predicted to exhibit multiple low-energy excited 0+ states attributed to neutron and proton excitations across both the N=40 and Z=28 shell gaps. In Ni68, the three observed 0+ states have been interpreted in terms of triple shape coexistence between spherical, oblate, and prolate deformed shapes. In the present work a new (02+) state at an energy of 1567 keV has been discovered in Ni70 by using β-delayed, γ-ray spectroscopy following the decay of Co70. The precipitous drop in the energy of the prolate-deformed 0+ level between Ni68 and Ni70 with the addition of two neutrons compares favorably with results of Monte Carlo shell-model calculations carried out in the large fpg9/2d5/2 model space, which predict a 02+ state at 1525 keV in Ni70. The result extends the shape-coexistence picture in the region to Ni70 and confirms the importance of the role of the tensor component of the monopole interaction in describing the structure of neutron-rich nuclei.

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  • Received 15 June 2015
  • Revised 9 September 2015
  • Corrected 28 December 2015

DOI:https://doi.org/10.1103/PhysRevC.92.061302

©2015 American Physical Society

Corrections

28 December 2015

Erratum

Publisher's Note: New low-energy 0+ state and shape coexistence in Ni70 [Phys. Rev. C 92, 061302(R) (2015)]

C. J. Prokop, B. P. Crider, S. N. Liddick, A. D. Ayangeakaa, M. P. Carpenter, J. J. Carroll, J. Chen, C. J. Chiara, H. M. David, A. C. Dombos, S. Go, J. Harker, R. V. F. Janssens, N. Larson, T. Lauritsen, R. Lewis, S. J. Quinn, F. Recchia, D. Seweryniak, A. Spyrou, S. Suchyta, W. B. Walters, and S. Zhu
Phys. Rev. C 93, 019901 (2016)

Authors & Affiliations

C. J. Prokop1,2,*, B. P. Crider1, S. N. Liddick1,2, A. D. Ayangeakaa3, M. P. Carpenter3, J. J. Carroll4, J. Chen1, C. J. Chiara5, H. M. David3,†, A. C. Dombos1,6, S. Go7, J. Harker3,8, R. V. F. Janssens3, N. Larson1,2, T. Lauritsen3, R. Lewis1,2, S. J. Quinn1,6, F. Recchia9, D. Seweryniak3, A. Spyrou1,6, S. Suchyta10, W. B. Walters8, and S. Zhu3

  • 1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
  • 2Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA
  • 3Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 4U.S. Army Research Laboratory, Adelphi, Maryland 20783, USA
  • 5Oak Ridge Associated Universities Fellowship Program, U.S. Army Research Laboratory, Adelphi, Maryland 20783, USA
  • 6Department of Physics, Michigan State University, East Lansing, Michigan 48824, USA
  • 7Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 8Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
  • 9Dipartimento di Fisica e Astronomia, Università degli Studi di Padova, I-35131 Padova, Italy
  • 10Department of Nuclear Engineering, University of California Berkeley, Berkeley, California 94720, USA

  • *prokop@nscl.msu.edu
  • Present address: GSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, Germany.

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Vol. 92, Iss. 6 — December 2015

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