https://hdl.handle.net/1721.1/150955 Tue, 07 Apr 2026 10:07:16 GMT 2026-04-07T10:07:16Z https://hdl.handle.net/1721.1/163371 The Wafold: A Theory of Spacetime Termination Inside Black Holes Viaña, Javier This article introduces a proposal for a novel conceptual interpretation of black holes in which spacetime can terminate on a curvature-triggered hypersurface. When curvature reaches a critical limit, the three-dimensional spatial geometry is proposed to undergo a dimensional compression into a thin, curved boundary identified as the wafold. Beyond this, spacetime no longer continues; the manifold itself comes to an end. All mass-energy and information would then be confined to the wafold, forming a structure consistent with the external Schwarzschild geometry and the Bekenstein-Hawking entropy law. We outline a possible Dimensional Conversion Law that could govern this phenomenon, and discuss the conservation, causal, and thermodynamic implications of the wafold at a conceptual level. This work should be regarded as a hypothesis-generating perspective, not a complete theory. Its purpose is to motivate further mathematical and physical inquiry. Wed, 22 Oct 2025 00:00:00 GMT https://hdl.handle.net/1721.1/163371 2025-10-22T00:00:00Z https://hdl.handle.net/1721.1/163175 The Boundawall: A Proposal on the Nature of Black Holes Viaña, Javier This research suggests a new interpretation of black holes in which the event horizon represents the termination of physical reality. In this view, when curvature approaches a critical threshold, the three-dimensional spatial geometry may undergo a dimensional compression into a two-dimensional manifold—the boundawall—that preserves gravitational continuity while preventing further causal evolution. Inside this surface, spacetime would cease to exist. All mass-energy and information would then be confined to the boundawall, forming a structure consistent with the external Schwarzschild geometry and the Bekenstein-Hawking entropy law. We outline a possible Dimensional Conversion Law that could govern this phenomenon, and discuss the conservation, causal, and thermodynamic implications of the boundawall. Finally, we comment on potential observational consistency and on limited predictions such as surface-mode signatures. In this theory, the event horizon is viewed not merely as a limit of observation, but as a potential boundary/wall of existence itself. Wed, 15 Oct 2025 00:00:00 GMT https://hdl.handle.net/1721.1/163175 2025-10-15T00:00:00Z