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Meson Dynamics and the Nuclear Many-Body Problem. I. The Free-Nucleon Problem

W. D. Brown*, R. D. Puff, and L. Wilets

  • University of Washington, Seattle, Washington 98105

  • *Present address: Department of Physics and Astronomy, and Center for Theoretical Physics, University of Maryland, College Park, Maryland.

Phys. Rev. C 2, 331 – Published 1 August, 1970

DOI: https://doi.org/10.1103/PhysRevC.2.331

Abstract

Relativistic nucleon-meson field theory is cast in a form appropriate to the nuclear many-body problem. Martin-Schwinger thermodynamic Green's functions are employed. The n-nucleon Green's functions satisfy a set of coupled equations which is formally identical to those of the usual potential many-body problem. Here, however, the two-body potential is replaced by a time-dependent interaction in which the mesons are formally eliminated in favor of higher-order nucleon correlations. A general program of increasing complexity for obtaining approximate solutions to the equations is discussed. It is necessary to solve the "vacuum" (one-, two-, etc., nucleon propagator) first. This has been done in the "Hartree-Fock" approximation which sums all diagrams containing a single continuous nucleon line with all possible uncrossed π and ω meson lines. Peaks in the spectral function are identified with masses of known N* resonances. The appearance of ghost states, which arise in the process of mass and wave-function renormalization, is discussed. The resultant Green's function is used to calculate the magnetic moment of the nucleon, yielding a significantly better isovector component of the magnetic moment than the usual perturbation theory, although the isoscalar component is poor in both cases.

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