N=16 subshell closure from stability to the neutron drip line

A. Obertelli, S. Péru, J. -P. Delaroche, A. Gillibert, M. Girod, and H. Goutte
Phys. Rev. C 71, 024304 – Published 7 February 2005

Abstract

The Hartree-Fock-Bogoliubov method implemented with the Gogny-D1S force and used in a systematic study of the even-even N=16 isotones from stability to the neutron drip line strongly suggests that a subshell gap, approximately 4 MeV wide, is opening at N=16. The first 2+ levels as well as B(E2;0gs+2+) reduced E2 transition probabilities have also been predicted in configuration mixing and standard random phase approximation calculations using D1S. These results compare favorably with experimental information available for the Z=1018 nuclei and with expectations for O24 properties. They also fully support our mean-field predictions, namely that N=16 is a spherical magic number at the oxygen neutron drip line.

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  • Received 17 November 2003

DOI:https://doi.org/10.1103/PhysRevC.71.024304

©2005 American Physical Society

Authors & Affiliations

A. Obertelli1, S. Péru2, J. -P. Delaroche2, A. Gillibert1, M. Girod2, and H. Goutte2

  • 1CEA-Saclay, DSM/DAPNIA/SPhN, F-91191 Gif-sur-Yvette, France
  • 2CEA/DIF/DPTA/SPN, Boîte Postale 12, F-91680 Bruyères-le-Chátel, France

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Vol. 71, Iss. 2 — February 2005

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