Role of retardation in 3-D relativistic equations

dc.creatorLahiff, A. D.
dc.creatorAfnan, I. R.
dc.date1997-08-20
dc.date.accessioned2026-07-07T11:11:19Z
dc.date.available2026-07-07T11:11:19Z
dc.descriptionEqual-time Green's function is used to derive a three-dimensional integral equation from the Bethe-Salpeter equation. The resultant equation, in the absence of anti-particles, is identical to the use of time-ordered diagrams, and has been used within the framework of $ϕ^2σ$ coupling to study the role of energy dependence and non-locality when the two-body potential is the sum of $σ$-exchange and crossed $σ$ exchange. The results show that non-locality and energy dependence make a substantial contribution to both the on-shell and off-shell amplitudes.
dc.description17 pages, RevTeX; 8 figures. Accepted for publication in Phys. Rev. C56 (Nov. 97)
dc.identifierhttps://arxiv.org/abs/nucl-th/9708037
dc.identifierhttp://arxiv.org/abs/nucl-th/9708037
dc.identifierPhys.Rev.C56:2387-2395,1997
dc.identifierdoi:10.1103/PhysRevC.56.2387
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191059
dc.subjectNuclear Theory
dc.titleRole of retardation in 3-D relativistic equations
dc.typetext

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