The Quantum Model of Spinning Black Holes

Abstract

We propose a quantum model of spinning black holes with the integrable ring singularities. For the charged Kerr-Newman quantum metric, the complete regularization takes place at fixing of the maximal (cut-off) energy of gravitons, $k_{UV}^{reg}=\hslash c/R_S^{reg}$.The domains of existence of one, two and several event horizons $r_q$ are shown depending on the parameters of modified Kerr and Kerr-Newman metrics.

arXiv comment15 pages, 2 figures, 1 table

References in corpus (8)

• New black holes in the brane-world?
• Gravitational decoupling for axially symmetric systems and rotating black holes
• Bound states and decay times of fermions in a Schwarzschild black hole background
• Non-Existence of Time-Periodic Solutions of the Dirac Equation in an Axisymmetric Black Hole Geometry
• Non-Existence of Time-Periodic Solutions of the Dirac Equation in a Reissner-Nordstrom Black Hole Background
• Bound states of the Dirac equation on Kerr spacetime
• Quantum rotating black holes
• Quantum mechanics of stationary states of particles in a space-time of classical black holes