White-Hole Emergence as Stabilized Routing: Black-Hole → White-Hole Networks in the ψ₀–OCM Framework

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Authors: John Francis Osborne
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Abstract

Black holes are commonly described as one-way gravitational sinks in which matter and energy irreversibly disappear. This view raises long-standing conceptual problems concerning information loss, conservation, and the continuity of physical processes. Within the ψ₀–OCM (Osborne Cosmological Model), gravitational collapse is not interpreted as destruction. Instead, black holes function as routing nodes within a broader redistribution architecture. Energy and structure transition across higher-dimensional boundaries and re-emerge as stabilized outflow structures that, in this framework, are interpreted as white-hole-like dynamics. The outflow is not a reversal of collapse, but a continuation of the same process under different boundary conditions. This paper develops the conceptual structure of routing and white-hole emergence, presenting stability considerations at a qualitative level and clarifying how routing replaces the notion of terminal singularities. The emphasis is conceptual rather than derivational: formal redistribution equations, stability operators, and internal node mechanics are deliberately withheld for deeper technical work. Routing also provides a natural pathway for outflow channels that do not couple electromagnetically, forming conceptual precursors to the dark sector — a subject deferred to later papers. The objective of this work is to establish the existence, coherence, and motivation for routing within ψ₀–OCM, positioning black holes not as endpoints, but as active interfaces in a broader redistribution network.

Fields of Study & Subjects

Cosmology and Gravitation Theories Pulsars and Gravitational Waves Research Black Holes and Theoretical Physics

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
3 January 2026
Language
EN