2.1 Proof of Refined Quantum Hill Theory in Proposed Radial Eigenstates
A nanoanalogue model of Kerr-Newman black holes was created to quantify energy states in quantum sciences around certain systems. Similarly to previous black hole simulations, such as the Blandford-Znajek jet program, the simulation ran expected according to classical dynamics. However, in light of recent research in quantum wells, theories on material accumulation around a black hole due to spin rates was theorized.
Furthermore, I have hypothesized that the accumulation of mass around a spinning black hole is comparable to the material accumulation within quantum wells. The mass rate spin of crystalline and gaseous substances around a black hole creates a similar resonance to that of a quantum well, more importantly. The criticality of this study lies in further implications that super-radiant physics holds for nuclear and applied elementary particle physics.
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