Investigates centripetal forces at a Schwarzschild black hole's event horizon, suggesting new observer frameworks.
**Version 2.0 Updates & Major Revisions:** * **Resolved Dimensional Inconsistency:** Fixed the mechanical unit mismatch in the previous version by formalizing the scaling factor with a mathematically rigorous squared Lorentz factor (γ²), ensuring the final output is strictly in Newtons (kg·m/s²). * **Introduced Dual-Framework Observer Model:** Resolved the boundary limitation at infinity (r → ∞) by branching the theory into two distinct reference frames: 1. *Historical Progenitor Framework:* Maps the inertial memory of the pre-collapse star (ω_past). 2. *Asymptotic Far-Field Framework:* Aligns with Einstein's General Relativity (ω_far) where required force trends to infinity at the horizon. * **Inter-Framework Linkage:** Formulated a direct mathematical transformational ratio linking the two observer frequencies, proving a non-linear topological breakdown at the event horizon (r = R_B).
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Jai Pandey (2026) studied this question.
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