Magnetic rotation and quasicollective structures in 58Fe: Influence of the νg9/2 orbital

D. Steppenbeck, R. V. F. Janssens, S. J. Freeman, M. P. Carpenter, P. Chowdhury, A. N. Deacon, M. Honma, H. Jin, T. Lauritsen, C. J. Lister, J. Meng, J. Peng, D. Seweryniak, J. F. Smith, Y. Sun, S. L. Tabor, B. J. Varley, Y.-C. Yang, S. Q. Zhang, P. W. Zhao, and S. Zhu
Phys. Rev. C 85, 044316 – Published 16 April 2012

Abstract

The structure of 58Fe was investigated at Gammasphere using 48Ca(13,14C,xn) fusion-evaporation reactions at a beam energy of 130 MeV. The level scheme has been revised and extended to J17 and an excitation energy of 16.6 MeV. Regular band structures consisting of low-energy ΔJ=1 transitions have been observed at moderate spin (J8–15) and are candidates for magnetic rotational bands. Self-consistent tilted-axis-cranking calculations within a relativistic mean-field theory were applied to investigate these bands and were found to reproduce the experimental results well. In other parts of the level scheme, quasirotational bands composed of stretched-E2 transitions have been extended to high spin, and other new bands have been identified. Positive-parity experimental states were compared to predictions of the spherical shell model using the GXPF1A, KB3G, and FPD6 effective interactions in the fp model space. The projected shell model, with a deformed quasiparticle basis including the neutron νg9/2 orbital, was applied to interpret regular ΔJ=2 band structures that extend beyond the maximum spin available for π[(f7/2)2] ν[(p3/2f5/2p1/2)4] configurations and exhibit features characteristic of rotational alignment. It is clear that the νg9/2 intruder orbital plays a crucial role in describing the quasirotational structures in this nucleus, even starting as low as J5.

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  • Received 22 February 2012

DOI:https://doi.org/10.1103/PhysRevC.85.044316

©2012 American Physical Society

Authors & Affiliations

D. Steppenbeck1,*, R. V. F. Janssens2, S. J. Freeman3, M. P. Carpenter2, P. Chowdhury4, A. N. Deacon3,†, M. Honma5, H. Jin6, T. Lauritsen2, C. J. Lister2, J. Meng7, J. Peng8, D. Seweryniak2, J. F. Smith3,‡, Y. Sun6,9,10, S. L. Tabor11, B. J. Varley3, Y.-C. Yang6, S. Q. Zhang7, P. W. Zhao7, and S. Zhu2

  • 1RIKEN Nishina Center, 2-1, Hirosawa, Wako, Saitama 351-0198, Japan
  • 2Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 3Schuster Laboratory, University of Manchester, Manchester M13 9PL, United Kingdom
  • 4Department of Physics, University of Massachusetts Lowell, Lowell, Massachusetts 01854, USA
  • 5Center for Mathematical Sciences, Aizu University, Tsuruga, Ikki-Machi, Aizu-Wakamatsu, Fukushima 965-8580, Japan
  • 6Department of Physics, Shanghai Jiao-Tong University, Shanghai 200240, People's Republic of China
  • 7State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijing 100871, People's Republic of China
  • 8Department of Physics, Beijing Normal University, Beijing 100875, People's Republic of China
  • 9Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, People's Republic of China
  • 10Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37966, USA
  • 11Department of Physics, Florida State University, Tallahassee, Florida 32306, USA

  • *steppenbeck@riken.jp
  • Present address: Cargo Division, Rapsican Systems, Prospect Way, Victoria Business Park, Stoke-on-Trent ST8 7PL, United Kingdom.
  • Present address: Department of Physics, University of the West of Scotland, Paisley PA1 2BE, United Kingdom.

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Issue

Vol. 85, Iss. 4 — April 2012

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