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.File | Dimensione | Formato | |
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PhysRevC.83.061304.pdf
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