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| Format: | Recurso digital |
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Zenodo
2025
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| Online Access: | https://doi.org/10.5281/zenodo.17382930 |
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Table of Contents:
- <p> </p> <p>This work formulates the behavior of quantum fields in curved spacetime inside black holes, using standard quantum mechanics coupled with general relativity. Particles are treated as wavefunctions propagating in strongly curved metrics. Classical singularities are regularized by Planck-scale energy density limits. The framework predicts modifications to Hawking radiation, possible effects on galaxy rotation curves, and the convergence of the four fundamental forces under extreme curvature, providing a heuristic pathway toward unification without introducing additional fields.</p> <p>\end{abstract}</p> <p> </p>