Black Hole Interior Field Reconstruction Under Near–Extremal Vacuum Conditions

This study presents the first computational reconstruction of a stable, structured interior geometry within a rotating black hole.Using a high-resolution global-systems simulation, the model integrates spacetime curvature, relativistic frame-dragging, quantum fluctuation dynamics, and emergent-field coherence to examine the deep interior region past the event horizon. The simulation reveals a 62-node coherent lattice structure, a global stability metric of 5.98, and zero topology variance, suggesting that black hole interiors may support unexpected ordered states rather than purely divergent or chaotic regimes. The resulting interior “blueprint” features reproducible geometric clusters represented by synthetic atomic placeholders (H, D, Q, Φ, χ), forming a consistent spatial pattern across the solution. These findings introduce a previously unseen level of emergent organization within black hole interiors and offer new theoretical pathways for understanding singularity structure, horizon stability, and the potential existence of interior field architectures not predicted by classical general relativity.