Asymptotic and integral relationships between the functions associated with the unphysical and physical spectral functions of partial-wave amplitudes with l ≧ 1 for the scattering of spinless particles are developed. The results are used to show that: (a) The function associated with the unphysical singularities must have a closely limited asymptotic behavior if the dispersion relation is to be consistent. (b) The unphysical singularities determine precisely the leading asymptotic term in the function associated with the physical cut and in the absence of unphysical singularities, there can be no scattering. (c) In many cases, the unphysical singularities determine the asymptotic limits of the transmission factor and the real part of the phase shift. (d) If the transmission factor goes to zero (maximal inelasticity), the rate at which it approaches this limit is sometimes bounded by a known function. In these cases, the unphysical singularities and the transmission factor together determine the leading asymptotic term of the phase shift. (e) In some situations, a sign inconsistency in the asymptotic constraints implies the existence of poles in any N D solution with residues whose signs prevent their interpretation as bound states. These poles are then “ghosts.” (f) In an exact partial-wave dispersion relation, at least when l ≧ 2, there is no simple way by which to determine, from the sign of the unphysical function at threshold or at infinity, whether the corresponding “force” is attractive or repulsive. This sign is fixed at these energies by general arguments. As a result of these constraints, one can conclude that the usual approximations of the unphysical cut in terms of the singularities of pole diagrams have a chance of satisfying consistency requirements only for the s- and p-waves with spin zero and one particle exchanges. For p-waves, the exchange of a spin one particle is required. Certain rapidly convergent integral identities are developed which can be used to test for the presence of ghosts or of bound states in N D solutions or to test the accuracy of solutions. Finally, the relativistic Chew-Low model is used to demonstrate numerically the importance of some of the restrictions obtained.
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