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

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

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Abstract

The neutron-rich 39S nucleus has been studied using binary grazing reactions produced by the interaction of a 215-MeV beam of 36S ions with a thin 208Pb 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 39S 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 39S that have the components in their wave functions corresponding to three neutrons in the 1ƒ7/2 orbital outside the N = 20 core have also been discussed within the context of the 0 ℏω shell-model calculations presented here.
Original languageEnglish
Article number024325
JournalPhysical Review C
Volume94
Issue number2
DOIs
Publication statusPublished - 17 Aug 2016

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