This paper develops a structural account of energy quantisation within the ψ₀-OCM (Osborne Cosmological Model). In this framework, particle-like excitations are treated as boundary-locked stabilization nodes characterised by boundary invariants and topological classes. Once a node is stabilized, the effective generator restricted to that sector admits a discrete spectrum, and these eigenmodes are interpreted as quanta. The analysis places stabilization prior to quantisation: discrete spectra are understood as properties of constrained redistribution flows rather than primitive assumptions. Quanta are not treated as fundamental building blocks, but as discrete modes supported by stabilized configurations, while the underlying ψ₀ redistribution remains continuous. The paper focuses on the structural logic of this ordering and does not attempt derivation of the full ψ₀ action, reconstruction of particle spectra, or numerical calibration. It aims to clarify how quantisation naturally emerges once stabilization is present within the broader ψ₀-OCM framework.
John Francis Osborne (Sun,) studied this question.
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