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Phys. Rev. C 73, 037309 (2006) [4 pages]

Spectroscopy of the odd-odd fp-shell nucleus 52Sc from secondary fragmentation

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A. Gade1, R. V. F. Janssens2, D. Bazin1, B. A. Brown1,3, C. M. Campbell1,3, M. P. Carpenter2, J. M. Cook1,3, A. N. Deacon4, D.-C. Dinca1,3, S. J. Freeman4, T. Glasmacher1,3, B. P. Kay4, P. F. Mantica1,5, W. F. Mueller1, J. R. Terry1,3, and S. Zhu2
1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
2Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
3Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
4Department of Physics and Astronomy, Schuster Laboratory, University of Manchester, Manchester M13 9PL, United Kingdom
5Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA

Received 17 January 2006; published 22 March 2006

The odd-odd fp-shell nucleus 52Sc was investigated using in-beam γ-ray spectroscopy following secondary fragmentation of a 55V and 57Cr cocktail beam. Aside from the known γ-ray transition at 674(5) keV, a new decay at Eγ=212(3) keV was observed. It is attributed to the depopulation of a low-lying excited level. This new state is discussed in the framework of shell-model calculations with the GXPF1, GXPF1A, and KB3G effective interactions. These calculations are found to be fairly robust for the low-lying level scheme of 52Sc irrespective of the choice of the effective interaction. In addition, the frequency of spin values predicted by the shell model is successfully modeled by a spin distribution formulated in a statistical approach with an empirical, energy-independent spin-cutoff parameter.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.73.037309
DOI:
10.1103/PhysRevC.73.037309
PACS:
23.20.Lv, 21.60.Cs, 25.70.Mn, 27.40.+z