PROBABLE STABILIZATION THEORY – Sequencing-Phase Effects in Light Propagation

This proposal investigates whether tiny, measurable “sequencing-phase” effects can be detected in the way light propagates across space and gravitational fields. While General Relativity predicts that gravitational lensing and Shapiro delays are achromatic (identical across wavelengths), this work explores the possibility of subtle wavelength-dependent or phase-like deviations that could signal new physics. The concept originates in Probable Stabilization Theory (PST), where time is modeled as a “linear ledger” and light’s phase is influenced by sequencing context. The paper outlines specific observational tests—from strong-lensing chromaticity to pulsar timing residuals—and provides falsifiable criteria, datasets, and methods. A positive detection would not only challenge current gravitational models but also provide empirical grounding for PST’s cosmological extensions. This hypothesis does not overturn General Relativity; instead, it uses GR’s predictions as the baseline and looks for small, second-order residuals in light propagation that GR does not explicitly model, ensuring all confirmed GR tests remain valid.