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Phys. Rev. C 38, 1861–1869 (1988)

Random phase approximation for light nuclei based on fully relativistic Hartree-Fock calculations

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P. G. Blunden and P. McCorquodale
TRIUMF, Vancouver, British Columbia, Canada V6T 2A3

Received 27 January 1988; published in the issue dated October 1988

The particle-hole spectra of light nuclei are examined in the self-consistent random phase approximation based on fully relativistic Hartree and Hartree-Fock models for the nuclear ground state. The particle-hole interaction is completely prescribed by the ground-state calculation. It includes σ, ω, ρ, and π meson exchanges, with σ and ω parameters adjusted to fit the bulk properties of nuclear matter. Differences between Hartree (no exchange) and Hartree-Fock (with exchange) predictions for the spectra are discussed.

© 1988 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.38.1861
DOI:
10.1103/PhysRevC.38.1861
PACS:
21.60.Jz