Phys. Rev. Lett. 92, 072502 (2004) [4 pages]Lowest Excitations in 56Ti and the Predicted N=34 Shell Closure
S. N. Liddick1,2, P. F. Mantica1,2, R. V. F. Janssens3, R. Broda4, B. A. Brown1,5, M. P. Carpenter3, B. Fornal4, M. Honma6, T. Mizusaki7, A. C. Morton1, W. F. Mueller1, T. Otsuka8, J. Pavan9, A. Stolz1, S. L. Tabor9, B. E. Tomlin1,2, and M. Wiedeking9 Received 9 September 2003; published 20 February 2004 Recent experimental characterization of the subshell closure at N=32 in the Ca, Ti, and Cr isotones has stimulated shell-model calculations that indicated the possibility that the N=34 isotones of these same elements could exhibit characteristics of a shell closure, namely, a high energy for the first excited 2+ level. To that end, we have studied the decay of 56Sc produced in fragmentation reactions and identified new γ rays in the daughter N=34 isotone 56Ti. The first 2+ level is found at an energy of 1127 keV, well below the expected position that would indicate the presence of an N=34 shell closure in 56Ti. ©2004 The American Physical Society
URL: http://link.aps.org/doi/10.1103/PhysRevLett.92.072502 [ Abstract | Previous article | Next article | Issue 7 ] |
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