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Phys. Rev. C 70, 034301 (2004) [5 pages]

Intermediate-energy Coulomb excitation of 52Fe

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K. L. Yurkewicz1,2, D. Bazin1, B. A. Brown1,2, C. M. Campbell1,2, J. A. Church1,2,*, D.-C. Dinca1,2, A. Gade1, T. Glasmacher1,2, M. Honma3, T. Mizusaki4, W. F. Mueller1, H. Olliver1,2, T. Otsuka5,6, L. A. Riley7, and J. R. Terry1,2
1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
2Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
3Center for Mathematical Sciences, University of Aizu, Tsuruga, Ikki-machi, Aizu-Wakamatsu, Fukushima 965-8580, Japan
4Institute of Natural Sciences, Senshu University, Higashimita, Tama, Kawasaki, Kanagawa 214-8580, Japan
5Department of Physics and Center for Nuclear Study, University of Tokyo, Hongo, Tokyo 113-0033, Japan
6RIKEN, Hirosawa, Wako-shi, Saitama 351-0198, Japan
7Department of Physics and Astronomy, Ursinus College, Collegeville, Pennsylvania 19426, USA

Received 9 February 2004; published 3 September 2004

The nucleus 52Fe with (N=Z=26) has been investigated using intermediate-energy Coulomb excitation in inverse kinematics. A reduced transition probability of B(E2;01+→21+)=817(102) e2 fm4 to the first excited 2+ state at 849.0(5) keV was deduced. The increase in excitation strength B(E2↑) with respect to the even-mass neighbor 54Fe (B(E2↑)=620(50) e2 fm4) agrees with shell-model expectations as the magic number N=28 is approached. This measurement completes the systematics of reduced transition strengths to the first excited 2+ state for the even-even N=Z nuclei up to mass A=56.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.70.034301
DOI:
10.1103/PhysRevC.70.034301
PACS:
27.40.+z, 25.70.De, 23.20.Lv, 23.20.Js

*Present address: Lawrence Livermore National Laboratory, Livermore, CA 94550.

 
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