Black Holes, Information, and Active Horizons: A Boundary-First Resolution Architecture in ψ₀–OCM

This manuscript develops a conceptual resolution architecture for the black-hole information problem within the ψ₀-OCM (Osborne Cosmological Model). In this framework, the horizon is not treated as a passive geometric surface but as an active redistributive boundary that organises the storage, transfer, and subsequent re-expression of information. The analysis sets out how, within this boundary-first perspective, • global evolution remains unitary,• Hawking-like radiation acquires information content through boundary-mediated couplings,• Page-curve behaviour arises from the evolving correlation structure, and• entropy is consistently accounted for across interior, boundary, and radiation sectors. The focus of the paper is the conceptual structure rather than detailed technical implementation. It establishes a coherent interpretive framework and records precedence for a redistribution-based treatment of black-hole information, while remaining compatible with established results in the regimes where conventional approaches are known to apply.