Gravitational Collapse and the Emergence of Cosmological Domains

This article develops the collapse-specialized branch of a broader personal model presented together with the companion paper On the Possible States of Space-Time. It explores gravitational collapse not as a path toward a physically meaningful singularity, but as a process approaching a maximum-density condition of space-time. Within this model, that limiting condition is associated with the emergence of a new temporal domain. This domain is not treated as initially empty, but as emerging already in a dense and extreme state linked to the collapse process itself. Matter crossing the horizon does not create the domain, but enters a regime that is already structurally opened and already physically extreme. The horizon is therefore interpreted not merely as a causal boundary, but as the interface between external collapse and the emergence of an internal cosmological domain. The purpose of the article is not to claim a finished theory, but to clarify and organize the collapse logic of a broader personal framework while remaining as close as possible to known gravitational physics and major observational constraints.