This work derives the nonlinear resonance behavior of the scalar sector of the Chronoflux framework directly from the governing field equations. Starting from the covariant Chronoflux action, the scalar–matter coupling is obtained and the response to rotating asymmetric mass distributions is analyzed. The resulting field equation reduces to a Mathieu-type system, producing parametric resonance and exponential amplification of the scalar energy density. The growth rate depends on the curvature of the coupling, the rotation frequency, and a geometric asymmetry factor. The mechanism predicts measurable energy exchange during spacecraft flybys and provides a falsifiable extension of the Chronoflux dynamics. The theory reduces to general relativity in the equilibrium limit and introduces no additional degrees of freedom beyond the established scalar sector.
Roy Herbert (Fri,) studied this question.