Abstract
A natural and unambiguous generalization of the boundary condition formalism previously proposed by this author is shown to result in a practical set of equations for describing relativistic three-particle scattering. These equations are exactly unitary, and can be readily generalized to the n-body case. Applied to the 0 and 1 states of the 3π system (I=0, 1, 2), they yield the π and ω as natural consequences of the ππ s- and p-wave phases; there are no spurious predictions. The equations appear ideal for relativistic data analysis.