Bethe-Goldstone Equation in Finite Nuclei

Joslyn R. Demos and Manoj K. Banerjee
Phys. Rev. C 5, 75 – Published 1 January 1972
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Abstract

Following Brandow's suggestion of setting QUQ=0, where U is the single-particle potential, the Bethe-Goldstone equation becomes Ψ=Φ[Q(QTQω]vΨ. This equation has been approximated by replacing Q with the Eden-Emery Pauli operator and by neglecting T^χ, where T^ is the off-diagonal part of the c.m. kinetic energy operator in the oscillator representation. Care has been taken to retain T^Φ, which is a large term. The approximate equation has been solved iteratively. It yields defect functions with the bulk of the effect of Q built in. Correction terms to our approximate results have been estimated. A very satisfactory feature of the present approach is that there is considerable cancellation between the so-called spectral and Pauli correction terms. The biggest correction term is χ|T^|χ, which can be as large as 0.5 MeV in the triplet even case.

  • Received 15 July 1971

DOI:https://doi.org/10.1103/PhysRevC.5.75

©1972 American Physical Society

Authors & Affiliations

Joslyn R. Demos* and Manoj K. Banerjee

  • Department of Physics and Astronomy, University of Maryland, College Park, Maryland 20742

  • *Present address: Institute 7, Stefan, Jamova 39, Ljubljana, pp. 199/IV Yugoslavia.

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Issue

Vol. 5, Iss. 1 — January 1972

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