Energy extraction from extremal charged black holes due to the BSW effect
arXiv:1207.5209 · doi:10.1103/PhysRevD.86.124039
Abstract
Two particles can collide in the vicinity of a rotating black hole producing the divergent energy in the centre of mass frame (the BSW effect). However, it was shown recently that an observer at infinity can register quite modest energies E and masses m which obey some upper bounds. In the present work the counterpart of the original BSW effect is considered that may occur even for radial motion of colliding particles near charged static black holes. It is shown that in some scenarios there are no upper bound on E and m . Thus the high-energetic and superheavy products of the BSW effect in this situation are, in principle, detectable at infinity.
7 pages
References in corpus (6)
- Charged Spinning Black Holes as Particle Accelerators
- Acceleration of particles by nonrotating charged black holes
- Collisional Penrose process near the horizon of extreme Kerr black holes
- Emergent Flux from Particle Collisions Near a Kerr Black Hole
- Upper limits of particle emission from high-energy collision and reaction near a maximally rotating Kerr black hole
- Energetics of particle collisions near dirty rotating extremal black holes: Banados-Silk-West effect versus Penrose process
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