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Dipole and quadrupole moments of Cu7378 as a test of the robustness of the Z=28 shell closure near Ni78

R. P. de Groote, J. Billowes, C. L. Binnersley, M. L. Bissell, T. E. Cocolios, T. Day Goodacre, G. J. Farooq-Smith, D. V. Fedorov, K. T. Flanagan, S. Franchoo, R. F. Garcia Ruiz, Á. Koszorús, K. M. Lynch, G. Neyens, F. Nowacki, T. Otsuka, S. Rothe, H. H. Stroke, Y. Tsunoda, A. R. Vernon, K. D. A. Wendt, S. G. Wilkins, Z. Y. Xu, and X. F. Yang
Phys. Rev. C 96, 041302(R) – Published 4 October 2017

Abstract

Nuclear spins and precise values of the magnetic dipole and electric quadrupole moments of the ground states of neutron-rich Cu7378 isotopes were measured using the Collinear Resonance Ionization Spectroscopy (CRIS) experiment at the CERN On-Line Isotope Mass Separator (ISOLDE) facility. The nuclear moments of the less exotic Cu73,75 isotopes were remeasured with similar precision, yielding values that are consistent with earlier measurements. The moments of the odd-odd isotopes, and 2978Cu (N=49) in particular, are used to investigate excitations of the assumed doubly magic Ni78 core through comparisons with large-scale shell-model calculations. Despite the narrowing of the Z=28 shell gap between N45 and N=50, the magicity of Z=28 and N=50 is restored toward Ni78. This is due to weakened dynamical correlations, as clearly probed by the present moment measurements.

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  • Received 27 May 2017
  • Revised 3 August 2017

DOI:https://doi.org/10.1103/PhysRevC.96.041302

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

R. P. de Groote1,*, J. Billowes2, C. L. Binnersley2, M. L. Bissell2, T. E. Cocolios1, T. Day Goodacre3, G. J. Farooq-Smith1, D. V. Fedorov4, K. T. Flanagan2, S. Franchoo5, R. F. Garcia Ruiz2, Á. Koszorús1, K. M. Lynch6, G. Neyens1,6, F. Nowacki7, T. Otsuka1,8,9,10, S. Rothe2,3, H. H. Stroke11, Y. Tsunoda10, A. R. Vernon2, K. D. A. Wendt12, S. G. Wilkins2, Z. Y. Xu1, and X. F. Yang1

  • 1KU Leuven, Instituut voor Kern- en Stralingsfysica, B-3001 Leuven, Belgium
  • 2School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
  • 3Engineering Department, CERN, CH-1211 Geneva 23, Switzerland
  • 4Petersburg Nuclear Physics Institute, 188350 Gatchina, Russia
  • 5Institut de Physique Nucléaire d'Orsay, F-91406 Orsay, France
  • 6Physics Department, CERN, CH-1211 Geneva 23, Switzerland
  • 7Institute Pluridisciplinaire Hubert Curien, 23 rue du Loess, F-67037 Strasbourg Cedex 2, France
  • 8Department of Physics, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
  • 9RIKEN Nishina Center, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
  • 10Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
  • 11Department of Physics, New York University, New York, New York 10003, USA
  • 12Institut für Physik, Johannes Gutenberg-Universität, D-55128 Mainz, Germany

  • *ruben.degroote@kuleuven.be

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Vol. 96, Iss. 4 — October 2017

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