The Informational Ontology of Black Holes in TAD-G: Causal Boundary Saturation and the Holographic Emergence of the Interior

The reconciliation of General Relativity and Quantum Mechanics at the extreme limits of gravitational collapse frequently requires a reassessment of assumptions regarding the continuity of the spacetime manifold. This paper extends the formalism of the Theory of Dynamic Gravitational Densification (TAD-G) to black hole physics, treating spacetime not as a continuous background field, but as the macroscopic manifestation of a discrete causal processing network. A topological derivation is presented, replacing the classical singular interior with a two-dimensional saturation boundary (the Bottleneck Horizon). The model demonstrates that the phase transition of baryonic matter into a two-dimensional condensate of Planck-scale qubits generates an area expansion proportional to the square of the mass (A ∝ M 2). Consequently, a decay in energy density per degree of freedom (Ep ∝ 1/M ) is observed, enabling the organic derivation of the Hawking Temperature from first principles of statistical mechanics. Furthermore, the AMPS Paradox is addressed by integrating the ER=EPR conjecture, positing that the three-dimensional metric within the black hole’s interior emerges strictly as a holographic projection of the computational complexity associated with quantum entanglement on the surface.