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dc.contributor.authorViaña, Javier
dc.date.accessioned2025-10-22T22:26:21Z
dc.date.available2025-10-22T22:26:21Z
dc.date.issued2025-10-22
dc.identifier.urihttps://hdl.handle.net/1721.1/163371
dc.description.abstractThis 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.en_US
dc.language.isoenen_US
dc.subjectBlack holesen_US
dc.subjectevent horizonen_US
dc.subjectdimensional transitionen_US
dc.subjectholographic scalingen_US
dc.subjectgravitational entropyen_US
dc.subjectconceptual proposalen_US
dc.titleThe Wafold: A Theory of Spacetime Termination Inside Black Holesen_US
dc.typeArticleen_US


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