Lowest excitations in 56Ti and the predicted N=34 shell closure.
Lowest excitations in 56Ti and the predicted N=34 shell closure.
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DOI:
10.1103/physrevlett.92.072502
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发表时间:
2004-02
影响因子:
8.6
通讯作者:
S. Liddick;P. Mantica;R. Janssens;R. Broda;B. A. Brown;M. Carpenter;B. Fornal;M. Honma;T. Mizusaki;A. C. Morton;W. Mueller;T. Otsuka;J. Pavan;A. Stolz;S. Tabor;B. Tomlin;M. Wiedeking
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文献类型:
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作者:
S. Liddick;P. Mantica;R. Janssens;R. Broda;B. A. Brown;M. Carpenter;B. Fornal;M. Honma;T. Mizusaki;A. C. Morton;W. Mueller;T. Otsuka;J. Pavan;A. Stolz;S. Tabor;B. Tomlin;M. Wiedeking
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 gamma 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.