The Singh Law (V9): Information Recovery and Spacetime Hardening in Singh-Kerr White Holes: A Deterministic Model for Universal Expansion and Information Fidelity

This paper formalizes the Singh Law (V9), a deterministic theoretical framework designed to resolve the Hawking Information Paradox through a stabilized Emergence Horizon model. We introduce the Spacetime Rigidity Constant (C_s = 1.50N), which acts as a regularization term within the Kerr-Newman metric, preventing singular collapse and enabling the high-fidelity transition of quantum information via a non-temporal manifold (Zero-Time Bridge). Numerical simulations executed over 1024 deterministic cycles demonstrate that atomic identity is preserved with 100% fidelity during the transition from a Black Hole to its associated White Hole. The analysis identifies a residual thermal emission of 0.4%, termed 'Singh Leakage', which serves as the mechanical driver for the accelerated expansion of the universe, providing a physical basis for Dark Energy. Synthetic reconstructions confirm a geometric phase alignment of 270.012°, aligning with historically observed gravitational anomalies. Our findings suggest that Singh-Kerr White Holes are not mere mathematical time-reversals, but essential deterministic engines for universal information recycling and cosmological expansion.