Structure of Si33 and the magicity of the N=20 gap at Z=14

S. Jongile, A. Lemasson, O. Sorlin, M. Wiedeking, P. Papka, D. Bazin, C. Borcea, R. Borcea, A. Gade, H. Iwasaki, E. Khan, A. Lepailleur, A. Mutschler, F. Nowacki, F. Recchia, T. Roger, F. Rotaru, M. Stanoiu, S. R. Stroberg, J. A. Tostevin, M. Vandebrouck, D. Weisshaar, and K. Wimmer
Phys. Rev. C 102, 024321 – Published 18 August 2020

Abstract

The structure of Si33 was studied by a one-neutron knockout reaction from a Si34 beam at 98.5 MeV/u incident on a Be9 target. The prompt γ rays following the de-excitation of Si33 were detected using the GRETINA γ-ray tracking array while the reaction residues were identified on an event-by-event basis in the focal plane of the S800 spectrometer at the National Superconducting Cyclotron Laboratory. The presently derived spectroscopic factor values, C2S, for the 3/2+ and 1/2+ states, corresponding to a neutron removal from the 0d3/2 and 1s1/2 orbitals, agree with shell model calculations and point to a strong N=20 shell closure. Three states arising from the more bound 0d5/2 orbital are proposed, one of which is unbound by about 930 keV. The sensitivity of this experiment has also confirmed a weak population of 9/2 and 11/21,2 final states, which originate from a higher-order process. This mechanism may also have populated, to some fraction, the 3/2 and 7/2 negative-parity states, which hinders a determination of the C2S values for knockout from the normally unoccupied 1p3/2 and 0f7/2 orbits.

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  • Received 11 March 2020
  • Revised 3 June 2020
  • Accepted 29 July 2020

DOI:https://doi.org/10.1103/PhysRevC.102.024321

©2020 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

S. Jongile1,2, A. Lemasson3,4, O. Sorlin3, M. Wiedeking2,5, P. Papka1,2, D. Bazin4, C. Borcea6, R. Borcea6, A. Gade4, H. Iwasaki4, E. Khan8, A. Lepailleur3, A. Mutschler7,3, F. Nowacki9, F. Recchia4, T. Roger3, F. Rotaru6, M. Stanoiu6, S. R. Stroberg4,10, J. A. Tostevin11, M. Vandebrouck7,3, D. Weisshaar4, and K. Wimmer12,13,4

  • 1Stellenbosch University, Private Bag X1, Matieland, Stellenbosch 7602, South Africa
  • 2iThemba LABS, PO Box 722, Somerset West 7129, South Africa
  • 3Grand Accélérateur National d'Ions Lourds (GANIL), CEA/DRF - CNRS/IN2P3, B. P. 55027, F-14076 Caen Cedex 5, France
  • 4Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824-1321, USA
  • 5School of Physics, University of the Witwatersrand, Johannesburg 2050, South Africa
  • 6IFIN-HH, P. O. Box MG-6, 76900 Bucharest-Magurele, Romania
  • 7Institut de Physique Nucléaire, IN2P3-CNRS, F-91406 Orsay Cedex, France
  • 8IJCLab, Université Paris-Saclay, CNRS/IN2P3, 91405 Orsay Cedex, France
  • 9Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
  • 10TRIUMF, 4004 Westbrook Mall, Vancouver, British Columbia, Canada V67 2A3
  • 11Department of Physics, University of Surrey, Guildford, Surrey GU2 7XH, United Kingdom
  • 12Department of Physics, The University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
  • 13Department of Physics, Central Michigan University, Mt. Pleasant, Michigan 48859, USA

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Vol. 102, Iss. 2 — August 2020

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