Particle motion and collisions around rotating regular black hole
arXiv:1407.3697 · doi:10.1007/s10509-015-2289-4
Abstract
The neutral particle motion around rotating regular black hole that was derived from the Ayón-Beato-García black hole solution by the Newman-Janis algorithm in the preceding paper [Phys. Rev. D 89, 104017, (2014)] has been studied. The dependencies of the ISCO (innermost stable circular orbits along geodesics) and unstable orbits on the value of the electric charge of the rotating regular black hole have been shown. Energy extraction from the rotating regular black hole through various processes has been examined. We have found expression of the center of mass energy for the colliding neutral particles coming from infinity, based on the BSW (Baňados-Silk-West) mechanism. The electric charge of rotating regular black hole decreases the potential of the gravitational field and the particle needs less bound energy at the circular geodesics. This causes the increase of efficiency of the energy extraction through BSW process in the presence of the electric charge from rotating regular black hole. It has been shown that the efficiency of the energy extraction from the rotating regular black hole via the Penrose process decreases with the increase of the electric charge and is smaller with compare to 20.7% which is the value for the extreme Kerr black hole with the specific angular momentum .
10 pages, 8 figures, 2 tables
References in corpus (6)
- Rotating regular black holes
- Generating rotating regular black hole solutions without complexification
- Rotating Regular Black Hole Solution
- Collisional Penrose process near the horizon of extreme Kerr black holes
- Penrose Process in Kerr-Taub-NUT Spacetime
- Rotating non-Kerr black hole and energy extraction