Spectroscopic factors in the N=20 island of inversion: The Nilsson strong-coupling limit

A. O. Macchiavelli, H. L. Crawford, C. M. Campbell, R. M. Clark, M. Cromaz, P. Fallon, M. D. Jones, I. Y. Lee, A. L. Richard, and M. Salathe
Phys. Rev. C 96, 054302 – Published 2 November 2017

Abstract

Spectroscopic factors, extracted from one-neutron knockout and Coulomb dissociation reactions, for transitions from the ground state of Mg33 to the ground-state rotational band in Mg32, and from Mg32 to low-lying negative-parity states in Mg31, are interpreted within the rotational model. Associating the ground state of Mg33 and the negative-parity states in Mg31 with the 32[321] Nilsson level, the strong coupling limit gives simple expressions that relate the amplitudes (Cj) of this wave function with the measured cross sections and derived spectroscopic factors (Sj). To obtain a consistent agreement with the data within this framework, we find that one requires a modified 32[321] wave function with an increased contribution from the spherical 2p3/2 orbit as compared to a standard Nilsson calculation. This is consistent with the findings of large-scale shell model calculations and can be traced to weak binding effects that lower the energy of low- orbitals.

  • Figure
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  • Received 10 July 2017

DOI:https://doi.org/10.1103/PhysRevC.96.054302

©2017 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

A. O. Macchiavelli1, H. L. Crawford1, C. M. Campbell1, R. M. Clark1, M. Cromaz1, P. Fallon1, M. D. Jones1, I. Y. Lee1, A. L. Richard2, and M. Salathe1

  • 1Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
  • 2Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA

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Vol. 96, Iss. 5 — November 2017

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