Yrast states in the neutron-rich (41)S nucleus have been studied using binary grazing reactions produced by the interaction of a 215-MeV beam of (36)S ions with a thin (208)Pb target. The magnetic spectrometer, PRISMA, and the gamma-ray array, CLARA, were used in the measurements. gamma-ray transitions of energy 449 and 638 keV were observed. Results from published intermediate-energy Coulomb excitation measurements in combination with those from the present work have led to the construction of a new (41)S level scheme. Proposed J(pi) values are based on experimental observation and on model-dependent arguments. The level scheme and published electromagnetic transition probabilities are discussed within the context of state-of-art shell-model calculations using the SDPF-U effective interaction. In contrast with the excellent agreement observed in earlier published work, here there are significant discrepancies between experiment and the results of shell-model calculations.

Collectivity in (41)S

POLLAROLO, Giovanni;
2011-01-01

Abstract

Yrast states in the neutron-rich (41)S nucleus have been studied using binary grazing reactions produced by the interaction of a 215-MeV beam of (36)S ions with a thin (208)Pb target. The magnetic spectrometer, PRISMA, and the gamma-ray array, CLARA, were used in the measurements. gamma-ray transitions of energy 449 and 638 keV were observed. Results from published intermediate-energy Coulomb excitation measurements in combination with those from the present work have led to the construction of a new (41)S level scheme. Proposed J(pi) values are based on experimental observation and on model-dependent arguments. The level scheme and published electromagnetic transition probabilities are discussed within the context of state-of-art shell-model calculations using the SDPF-U effective interaction. In contrast with the excellent agreement observed in earlier published work, here there are significant discrepancies between experiment and the results of shell-model calculations.
2011
83
061304
-
Z. M. Wang;R. Chapman;F. Haas;X. Liang;F. Azaiez;B. R. Behera;M. Burns;L. Corradi;D. Curien;A. N. Deacon;Z. Dombradi;E. Farnea;E. Fioretto;A. Gadea;A. Hodsdon;F. Ibrahim;A. Jungclaus;K. Keyes;V. Kumar;A. Latina;N. Marginean;G. Montagnoli;D. R. Napoli;J. Ollier;D. O'Donnell;A. Papenberg;G. Pollarolo;M. D. Salsac;F. Scarlassara;J. F. Smith;K. M. Spohr;M. Stanoiu;A. M. Stefanini;S. Szilner;M. Trotta;D. Verney
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/98156
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