Reduced transition probabilities to the first 2 + state in 52 , 54 , 56 Ti and development of shell closures at N = 32 , 34
نویسندگان
چکیده
D.-C. Dinca,1,2 R. V. F. Janssens,3 A. Gade,2 D. Bazin,2 R. Broda,4 B. A. Brown,1,2 C. M. Campbell,1,2 M. P. Carpenter,3 P. Chowdhury,3,5 J. M. Cook,1,2 A. N. Deacon,6 B. Fornal,4 S. J. Freeman,6 T. Glasmacher,1,2 M. Honma,7 F. G. Kondev,8 J.-L. Lecouey,2 S. N. Liddick,2,9 P. F. Mantica,2,9 W. F. Mueller,2 H. Olliver,1,2 T. Otsuka,10 J. R. Terry,1,2 B. A. Tomlin,2,9 and K. Yoneda2 1Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824 2National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824 3Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 4Institute of Nuclear Physics, Polish Academy of Sciences, PL-31342 Cracow, Poland 5University of Massachusetts Lowell, Lowell, Massachusetts 01854 6Department of Physics and Astronomy, Schuster Laboratory, University of Manchester, Manchester M13 9PL, United Kingdom 7Center for Mathematical Sciences, University of Aizu, Tsuruga, Ikki-machi, Aizu-Wakamatsu, Fukushima 965-8580, Japan 8Nuclear Engineering Division, Argonne National Laboratory, Argonne, Illinois 60439 9Department of Chemistry, Michigan State University, East Lansing, Michigan 48824 10Department of Physics and Center for Nuclear Study, University of Tokyo, Hongo, Tokyo 113-0033, Japan and RIKEN, Hirosawa, Wako-shi, Saitama 351-0198, Japan (Received 8 November 2004; published 15 April 2005)
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