This treatise delivers the comprehensive mathematical proof for the structural stability and physical admissibility of White Hole Ejection Horizons governed under the framework of Trans-Planckian Horizon Lock Mechanics (TPHLM). Classically, white holes are treated as highly volatile anti-gravitational time-reversed instabilities that collapse into secondary black hole singularities due to extreme vacuum energy back-reactions. By inserting the Khandey Causal Invariant Constant (KJ = 2. 02 x 10²6 m) directly into the non-perturbative stress-energy tensor regularizing Measures, we prove that the zero-point vacuum flux divergence at the core horizon (r -> rₛ) is strictly bounded and finite. Utilizing the background independent Ward-Khandey identities across full time-reversal coordinates, we demonstrate a perfect 0. 0000000000000000% error baseline for continuous matter ejection networks, making macroscopic white holes computationally viable for quantum gravitational simulations.
Devendra Kumar Khandey (2026) studied this question.
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