This preprint introduces an original prediction within the CCEGA (Cosmic Curvature Emergence from Gravitational Adaptation) framework. It proposes that quantum fluctuations of curvature generate self-stabilizing gravitational structures in the centers of galaxies, altering the standard understanding of supermassive black holes (SMBHs). Instead of collapsing into singularities, these regions exhibit a dynamically emergent curvature field, which could explain certain observational anomalies such as larger-than-expected black hole shadows, unstable accretion disk structures, and deviations in gravitational lensing.
The study presents a modified Kerr-like metric incorporating oscillatory curvature effects and outlines observational signatures that can be tested with instruments like the Event Horizon Telescope (EHT), Chandra, XMM-Newton, and JWST. This prediction provides a testable alternative to singularity-based black hole models, offering new perspectives on high-energy astrophysics and quantum gravity.
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