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| Format: | Recurso digital |
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Zenodo
2026
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| Online adgang: | https://doi.org/10.5281/zenodo.18972727 |
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Indholdsfortegnelse:
- <p>This article continues the conceptual exploration initiated in the work <em>Gravitational Collapse and the Possible Emergence of Daughter Universes</em> (DOI: 10.5281/zenodo.18970318), in which a speculative framework was proposed suggesting that gravitational collapse inside black holes could potentially lead to the emergence of new cosmological regions once a maximum space-time density is reached.</p> <p>The present work focuses on a more fundamental aspect of this idea by examining the possible geometric and physical nature of space-time itself. Rather than treating space-time only as a mathematical background for physical processes, the article explores the possibility that space-time may possess an intrinsic geometric structure whose properties could evolve under strong gravitational conditions.</p> <p>Within this perspective, matter and energy may be interpreted as different configurations of an underlying geometric fabric, while gravitational phenomena correspond to variations in curvature and structural organization. The article introduces the notion of an effective geometric density of space-time and discusses the hypothesis that space-time might possess a finite maximum density. If such a limit exists, it may imply the existence of different structural regimes of space-time, ranging from the classical gravitational regime described by general relativity to extreme high-curvature configurations.</p> <p>Particular attention is given to the interpretation of event horizons as possible geometric interfaces separating distinct regimes of space-time structure. A conceptual phase diagram is proposed to illustrate how increasing curvature and density could lead to transitions between these regimes.</p> <p>This work should be understood as a conceptual and exploratory theoretical reflection developed independently by the author. The author is not a professional physicist but an independent reader with a strong interest in cosmology and theoretical physics. The goal of the article is therefore not to present a definitive physical theory, but rather to organize and explore a set of personal ideas and questions about the structure of space-time and its possible role in gravitational collapse and cosmological evolution.</p> <p>As a consequence, the work may remain limited in terms of formalism or scientific rigor compared to academic standards. The manuscript may evolve through future revisions as the author continues to learn and refine the ideas presented. Constructive feedback, corrections, and suggestions from readers are very welcome.</p> <p> </p> <p>v2. Note: added a new section discussing possible multiple geometric deformation modes of space-time (curvature and torsion) within the conceptual framework of the article.</p>