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Shell-Model Calculation for Masses 27, 28, and 29: General Methods and Specific Applications to Al27, Si28, and Si29

B. H. Wildenthal*

J. B. McGrory

  • Cyclotron Laboratory and Physics Department, Michigan State University, East Lansing, Michigan 48823

  • Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830

  • *Research supported in part by the National Science Foundation.
  • Research sponsored by the U. S. Atomic Energy Commission under contract with the Union Carbide Corporation.

Phys. Rev. C 7, 714 – Published 1 February, 1973

DOI: https://doi.org/10.1103/PhysRevC.7.714

Abstract

A shell-model calculation for A=27,28, and 29 nuclei has been carried out in a truncated 0d521s120d32 basis space with a modified-surface-δ-interaction Hamiltonian. A comparison of the calculated results for level energies, single-nucleon spectroscopic factors and E2 and M1 transition strengths in Al27, Si28, and Si29 with the corresponding experimental values indicates that a unified and quantitive explanation of nuclear structure around A=28 can be obtained via shell-model techniques.

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