Emergent Quantised Gravitational Behaviour from ψ₀ Redistribution and Partial Individuation

Standard physics successfully describes gravity classically throughGeneral Relativity and matter quantum mechanically, yet a unifiedmechanistic account of why gravity appears classical in most regimes andunder what conditions quantised behaviour should emerge remainsunresolved. This paper develops a ψ₀–OCM (Osborne Cosmological Model)framework in which quantised gravitational behaviour arises as anemergent consequence of discrete redistribution and partialindividuation within a generative ψ₀ substrate, rather than through thepostulation of a fundamental graviton field. The approach is empirically conservative: it preserves relativisticcausality, no-signalling, and the classical General Relativity limit undercoarse-graining. Quantised curvature behaviour is shown to arise inregimes where redistribution microstructure and stabilisation thresholdsremain unresolved, while classical gravity emerges as the effectivecoarse-grained description once individuation completes. The paperformalises this mechanism through structural postulates, reductionarguments, and regime-based theorems, and provides a constrained roadmapfor discriminating predictions without premature parameter commitments.