Abstract

This specification formalizes Asymmetric Horizon Rotational Compression (AHRC), a non-perturbative theoretical framework that resolves the mathematical infinity paradoxes (singularities) and informational lockouts inherent in standard general relativistic black hole metrics (e.g., the Kerr metric). Traditional astrophysics treats rotating collapsed mass metrics as infinite-density geometric singularities bounded by an un-passable event horizon. This framework creates a structural breakdown in causality and information conservation, causing the standard theoretical architecture to fracture under extreme energy densities.

AHRC systematically resolves this systemic failure by mapping the collapsed node not as an infinite point or ring mass, but as a localized, high-velocity torsional vortex spinning within a two-dimensional viscoelastic fluid membrane resting at absolute equilibrium (z=0) [1.1]. By analyzing the system through non-linear continuum mechanics, we prove that the immense angular momentum induces a localized shear-strain phase inversion at the apparent boundary [4.0]. This configuration transforms the catastrophic singularity into a highly compressed, stable, and pass-through macroscopic wave energy packet.

This brief details the continuous torsional fluid-substrate field equations, a production-ready Python simulation modeling horizon metric density scaling, a functional Cypher graph database architecture, and a comprehensive glossary of metrics.

Creative Commons License

Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.

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