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The Kerr–Newman Black Hole Solution as Strong Gravity for Elementary Particles

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Abstract

Analyzing the model of a spinning particle based on the over-rotating Kerr–Newman solution regularized by a supersymmetric bag model, we arrive at the conclusion that a unification of gravity with quantum theory is achieved in this model due to a strong topological influence of the Kerr spinning gravity which occurs on the Compton scale. We obtain that the correct formation of the nonperturbative bag model requires the use of the supersymmetric Landau–Ginzburg field model. We obtain that one of the most important gravitational phenomena in particle physics is the appearance of the quantum Wilson loop caused by the effect of frame-dragging related to the spin. Being located on the sharp border of the bag, the Wilson loop has a strong influence on the circular D-string structure located there.

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Notes

  1. We consider these loops as potentially possible Wilson loops. In many respects, the emergence of this series of closed loops \(C_{n}\) with the quantum phase increment \(2\pi n=\frac{1}{\hbar}\oint j_{\mu}A^{\mu}\) resembles the series of Bohr-Sommerfeld quantum orbits. Note that this is a purely classical effect, which is caused by the frame-dragging field near the border of the regularized KN solution. We see that the Kerr spinning gravity reproduces some elements of quantum theory on the classical level.

  2. This can explain the absence of classical radiation from an excited orientifold string.

  3. In string theory this peculiar point is called the orientifold plane.

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ACKNOWLEDGMENTS

I would like to thank M. Gürses, Yu.N. Obukhov and K. Stepaniantz for very kind information about the appearance of the article [5], and also all colleagues of the Theoretical Physics Laboratory of our Institute for useful discussions at different stages of this work. I also thank N. Arkani-Hamed for his kind response to the letter about this problem.

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  1. Theor. Phys. Lab., Nuclear Safety Institute, Russian Academy of Sciences, B. Tulskaya, 52, 115191, Moscow, Russia

    A. Burinskii

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Burinskii, A. The Kerr–Newman Black Hole Solution as Strong Gravity for Elementary Particles. Gravit. Cosmol. 26, 87–98 (2020). https://doi.org/10.1134/S020228932002005X

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