Relativistic field-theoretical approach to the inverse scattering problem

preprint2002arXivOpen access

Abstract

The inverse scattering problem for the relativistic three-dimensional equation (2Ep′−2Ep)<p′∣Ψp>=−∫V(t)d3p′′<p′′∣Ψp>\Bigl(2E_{\bf p'}-2E_{\bf p}\Bigr)<{\bf p'}|Ψ_{\bf p}>= -\int V(t)d^3{\bf p''}<{\bf p''}|Ψ_{\bf p}> with Ep=m2+p2E_{\bf p}=\sqrt{m^2+{\bf p}^2} and t=(Ep′−Ep′′)2−(p′−p′′)2t=\Bigl(E_{\bf p'}-E_{\bf p''}\Bigr)^2 -\Bigl({\bf p'}-{\bf p''}\Bigr)^2 is considered. The field-theoretical potential V(t)V(t) of this equation is constructed in the framework of the old perturbation theory. It contains all contributions of diagrams with intermediate off-mass shell particles. In particular, this potential reproduces the OBE Bonn model of the NNNN potential exactly.For the πNπN scattering it is generated by σ,ρ,ωσ,ρ, ω-meson exchange diagrams. The inverse scattering problem is solved by reduction of these relativistic equations to the standard Schrödinger equations (Δr+k2)<r∣ϕp>=−v(r)<r∣ϕk>\Bigl(Δ_{\bf r}+{\bf k}^2\Bigr)<{\bf r}|ϕ_{\bf p}>= - v({\bf r})<{\bf r}|ϕ_{\bf k}> with Ep=k2/2m+mE_{\bf p}={\bf k}^2/2m+m. The relation between the relativistic potential V(t)V(t) and its nonrelativistic representation v(r)v({\bf r}) is obtained.

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