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First in-beam gamma-ray study of the level structure of neutron-rich 39S

Authors :
Chapman, R.
Wang, Z. M.
Bouhelal, M.
Haas, F.
Liang, X.
Azaiez, F.
Behera, B. R.
Burns, M.
Caurier, E.
Corradi, L.
Curien, D.
Deacon, A. N.
Dombradi, Zs.
Farnea, E.
Fioretto, E.
Gadea, A.
Hodsdon, A.
Ibrahim, F.
Jungclaus, A.
Keyes, K.
Kumar, V.
Lunardi, S.
Marginean, N.
Montagnoli, G.
Napoli, D. R.
Nowacki, F.
Ollier, J.
O'Donnell, D.
Papenberg, A.
Pollarolo, G.
Salsac, M.-D.
Scarlassara, F.
Smith, J. F.
Spohr, K. M.
Stanoiu, M.
Stefanini, A. M.
Szilner, Suzana
Trotta, M.
Verney, D.
Publication Year :
2016

Abstract

The neutron-rich S39 nucleus has been studied using binary grazing reactions produced by the interaction of a 215-MeV beam of S36 ions with a thin Pb208 target. The magnetic spectrometer, PRISMA, and the γ-ray array, CLARA, were used in the measurements. Gamma-ray transitions of the following energies were observed: 339, 398, 466, 705, 1517, 1656, and 1724 keV. Five of the observed transitions have been tentatively assigned to the decay of excited states with spins up to (11/2−). The results of a state-of-the-art shell-model calculation of the level scheme of S39 using the SDPF-U effective interaction are also presented. The systematic behavior of the excitation energy of the first 11/2− states in the odd-A isotopes of sulfur and argon is discussed in relation to the excitation energy of the first excited 2+ states of the adjacent even-A isotopes. The states of S39 that have the components in their wave functions corresponding to three neutrons in the 1f7/2 orbital outside the N=20 core have also been discussed within the context of the 0 ℏω shell-model calculations presented here.

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.57a035e5b1ae..3edc1ca76f67273d831dd9b1c2276266