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| Autores principales: | , |
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| Formato: | Recurso digital |
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| Publicado: |
Zenodo
2025
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| Materias: | |
| Acceso en línea: | https://doi.org/10.5281/zenodo.16546176 |
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- <div> <div> <div> <div> <p>Abstract</p> <p>The presence of a central singularity within the Kerr-Newman metric is a well-established indication that General Relativity is incomplete at the quantum scale. This paper introduces a novel, non-singular solution to the Einstein-Maxwell equations, derived by introducing a physically motivated, higher-order curvature correction term. The analysis was performed using a novel methodology, the MOO Framework v1.0.0, which treats established physical theories as verifiable logical architectures, allowing for the deterministic propagation of new axiomatic assumptions. By augmenting the Einstein-Maxwell action with a hypothetical quantum gravity term that becomes significant only at extreme curvatures, we derive a modified Kerr-Newman solution. This new metric is regular everywhere, replacing the classical ring singularity with a finite, Planck-scale core structure. We demonstrate that this modification preserves the asymptotic properties of the original metric, remaining consistent with existing observational data. The most significant result of this regularized geometry is a unique, falsifiable prediction: the generation of a series of discrete, high-frequency "echoes" in the post-merger ringdown of gravitational waves, caused by reflections off the boundary of this Planck-scale core. This prediction provides a concrete observational target for next-generation gravitational wave detectors, offering a potential empirical test for this class of quantum gravity modifications.</p> </div> </div> </div> </div>