Microscopic calculations of the spectra of light nuclei

D. C. Zheng, B. R. Barrett, L. Jaqua, J. P. Vary, and R. J. McCarthy
Phys. Rev. C 48, 1083 – Published 1 September 1993
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Abstract

We perform large-space shell-model calculations for the low-lying energy spectra of a few light nuceli,4He, He5, Li6, and Li7, in a no-core model space with a realistic effective two-body interaction (Brueckner G matrix). Our G matrices are calculated for the Reid-soft-core potential in a harmonic-oscillator basis. Single-particle ‘‘-U’’ insertions are replaced by two-particle ‘‘-U’’ insertions and are included in the G-matrix calculations, which sum them to all orders. With the starting energy of the G matrix chosen to give approximately the experimental binding energy, we obtain nuclear energy spectra which are in reasonable agreement with experiment. We also investigate the dependence of our results on the size of the model space and on the harmonic-oscillator basis parameter (ħΩ).

  • Received 29 April 1993

DOI:https://doi.org/10.1103/PhysRevC.48.1083

©1993 American Physical Society

Authors & Affiliations

D. C. Zheng, B. R. Barrett, and L. Jaqua

  • Department of Physics, University of Arizona, Tucson, Arizona 85721

J. P. Vary

  • Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011
  • Institute for Theoretical Physics, University of Heidelberg, Heidelberg, Germany

R. J. McCarthy

  • Department of Physics, Kent State University, Ashtabula, Ohio 44004

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Vol. 48, Iss. 3 — September 1993

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