Phys. Rev. C 72, 044315 (2005) [8 pages]
Yrast structure of neutron-rich 53Ti
B. Fornal et al.
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B. Fornal1, S. Zhu2, R. V. F. Janssens2, M. Honma3, R. Broda1, B. A. Brown4,5, M. P. Carpenter2, S. J. Freeman2,6, N. Hammond2, F. G. Kondev7, W. Królas1,8, T. Lauritsen2, S. N. Liddick4,9, C. J. Lister2, S. Lunardi10, P. F. Mantica4,9, N. Marginean11, T. Mizusaki12, E. F. Moore2, T. Otsuka13,14, T. Pawłat1, D. Seweryniak2, B. E. Tomlin4,9, C. A. Ur10, I. Wiedenhöver2, and J. Wrzesiński1 1Institute of Nuclear Physics, Polish Academy of Sciences, PL-31342 Cracow, Poland
2Physics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
3Center for Mathematical Sciences, University of Aizu, Tsuruga, Ikki-machi, Aizu-Wakamatsu, Fukushima 965-8580, Japan
4National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
5Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
6Schuster Laboratory, University of Manchester, Manchester M13 9PL, United Kingdom
7Nuclear Engineering Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
8Joint Institute for Heavy Ion Research, Oak Ridge, Tennessee 37831, USA
9Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA
10Dipartimento di Fisica dell'Università di Padova, and INFN Sezione di Padova, I-35131 Padova, Italy
11INFN, Laboratori Nazionali di Legnaro, I-35020 Legnaro, Italy
12Institute of Natural Sciences, Senshu University, Higashimita, Tama, Kawasaki, Kanagawa 214-8580, Japan
13Department of Physics, University of Tokyo, Hongo, Tokyo 113-0033, Japan
14RIKEN, Hirosawa, Wako-shi, Saitama 351-0198, Japan
Received 22 June 2005; published 27 October 2005
γ rays from neutron-rich Ti nuclei in the vicinity of N=32 have been studied at Gammasphere using deep-inelastic reactions induced by 48Ca beams on thick 208Pb and 238U targets. The 53Ti yrast cascade was identified for the first time, and the location in energy of states with spin up to I = 21/2 was determined. The excitations of 53Ti provide new tests of effective interactions for full-pf-shell calculations. Comparisons between theory and experiment for the highest spin states in 53Ti favor the recently proposed GXPF1A interaction, which accounts for the appearance of a neutron subshell closure at N=32 in Ti isotopes as well as for the lack of a similar subshell closure at N=34, as predicted by earlier calculations with another interaction.
©2005 The American Physical Society
URL: http://link.aps.org/doi/10.1103/PhysRevC.72.044315
DOI: 10.1103/PhysRevC.72.044315
PACS: 21.60.Cs, 23.20.Lv, 27.40.+z, 25.70.Lm
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