Information Saturation and Geometric Information Encoding in the MBB-DI Framework

The black hole information paradox arises from the apparent conflict between singularity formation in classical general relativity and information-preserving evolution in quantum theory. In the standard Hawking picture, black hole evaporation appears approximately thermal, leading to the possibility of irreversible information loss. Building upon earlier MBB-DI (Multiple Big Bang -Domain Interaction) work on black-hole shell structure, halo-induced stabilization, Domain Interaction (DI) accumulation, and Quantum Bias of Spacetime (QBS), this paper develops a geometric-information interpretation in which information saturation can be achieved without requiring continued collapse toward a singularity. It is proposed that information is not fundamentally stored in matter or confined to horizon microstates, but is encoded in the evolving geometry of spacetime. A mathematical framework is developed in which information is represented through geometric degrees of freedom, including curvature, shell structure, halo structure, accumulated DI effects, and QBS-induced asymmetries. Geometric information conservation, Hawking-radiation correlations, and semiclassical information preservation are examined within a unified framework. Holographic entropy behavior and geometric-memory regimes emerge as limiting cases. Within this interpretation, black holes are viewed as extreme geometric information-encoding structures rather than information-destroying objects. The framework provides a unified perspective on information saturation, information preservation, spacetime memory, DI accumulation, and QBS within the broader MBB-DI cosmological framework.