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Phys. Rev. C 79, 034319 (2009) [6 pages]

Levels above the 19/2- isomer in 71Cu: Persistence of the N=40 neutron shell gap

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I. Stefanescu1,2,3, W. B. Walters1, R. V. F. Janssens2, N. Hoteling1,2, R. Broda4, M. P. Carpenter2, B. Fornal4, A. A. Hecht1,2, W. Krolas4,5, T. Lauritsen2, T. Pawlat4, D. Seweryniak2, J. R. Stone1,6, X. Wang2,7, A. Wöhr1,2, J. Wrzesinski4, and S. Zhu2
1Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742, USA
2Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
3Horia-Hulubei National Institute for Physics and Nuclear Engineering, P. O. Box MG-6, Bucharest, Romania
4Niewodniczanski Institute for Nuclear Physics, Krakow PL-31342, Poland
5Joint Institute for Heavy Ion Research, Oak Ridge, Tennessee 37831, USA
6Department of Physics, University of Oxford, OX1 3PU Oxford, United Kingdom
7Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA

Received 4 December 2008; published 26 March 2009

Two prompt γ rays of energies 2020 and 554 keV were observed in coincidence with delayed transitions depopulating the 19/2- isomer in the Z=29, N=42 71Cu nucleus. The newly identified transitions are proposed to deexcite the 4776- and 5330-keV levels above the 19/2- isomer. Based on the comparison with the low-lying positive-parity states observed in the Z=42, N=50 92Mo nucleus, spin and parity 23/2- are proposed for the 4776-keV level in 71Cu. The high-energy, 2020-keV transition is interpreted as arising from the breaking of the N=40 neutron core. Shell-model calculations with a 56Ni core reproduce the (23/2-)→(19/2-) gap well, suggesting that the 23/2- state is dominated by πp3/2ν((fp)10(g9/2)4) configurations. The present result constitutes further evidence supporting the view that the N=40 subshell closure persists in 71Cu, herewith challenging recent suggestions that the coupling of two or more proton or neutron quasiparticles induces a large polarization of the 68Ni core.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.79.034319
DOI:
10.1103/PhysRevC.79.034319
PACS:
23.20.Lv, 21.60.Cs, 27.50.+e, 23.35.+g