Published March 2009 | Version v1
Journal article

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

  • 1. Horia-Hulubei National Institute for Physics and Nuclear Engineering, P. O. Box MG-6, Bucharest (Romania)
  • 2. Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
  • 3. Department of Chemistry and Biochemistry, University of Maryland, College Park, Maryland 20742 (United States)
  • 4. Niewodniczanski Institute for Nuclear Physics, Krakow PL-31342 (Poland)
  • 5. Joint Institute for Heavy Ion Research, Oak Ridge, Tennessee 37831 (United States)
  • 6. Department of Physics, University of Oxford, OX1 3PU Oxford (United Kingdom)
  • 7. Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556 (United States)

Description

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

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
79
Journal Issue
3
Journal Page Range
p. 034319-034319.6
ISSN
0556-2813
CODEN
PRVCAN

Optional Information

Notes
(c) 2009 The American Physical Society