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| Autor principal: | |
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| Formato: | Recurso digital |
| Lenguaje: | inglés |
| Publicado: |
Zenodo
2026
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| Materias: | |
| Acceso en línea: | https://doi.org/10.5281/zenodo.20014389 |
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- <p>his work introduces κ-Theory, a nonlinear extension to gravitational dynamics in which collapse behavior depends not only on local energy density but on the structural intensity of its formation.</p> <p>The κ-term introduces a history-weighted correction proportional to density gradients, modifying collapse pathways in high-energy environments such as early-universe structure formation.</p> <p>Simulations demonstrate accelerated convergence relative to standard General Relativity, suggesting that overlapping density gradients bias structure formation before full separation.</p> <p>The framework implies a memory-dependent universe in which formation history affects present evolution without permitting causal reversal.</p> <p>Testable predictions, simulation boundaries, and cosmological implications are defined.</p>