Abstract
This paper presents an in-depth investigation of the super-Penrose process within Schwarzschild black holes, framed under the principles of Bell's theorem. By extending the classical Penrose mechanism and integrating quantum entanglement as described by Bell's theorem, we explore the feasibility of energy extraction near the event horizon through extreme collision conditions. The study incorporates a comprehensive analysis of both classical particle dynamics and quantum entangled states, highlighting the potential implications of quantum non-locality in black hole physics. Advanced mathematical formulations and physical models are employed to delineate the energy collision mechanisms under stringent conditions, evaluating the theoretical upper limits of energy extraction and their profound physical significance. The results underscore the enhanced efficiency of the super-Penrose process compared to its classical counterpart and provide novel insights into the interplay between quantum mechanics and general relativity in extreme astrophysical environments.



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