Bañados-Silk-West effect with nongeodesic particles: extremal horizons
arXiv:1307.0034 · doi:10.1103/PhysRevD.88.064036
Abstract
The Bañados-Silk-West (BSW) effect consists in the possibility to obtain arbitrarily large energy in the centre of mass frame of two colliding particles near the black hole horizon. One of the common beliefs was that the action of force on these particles (say, due to gravitational radiation) should necessarily restrict the growth of . We consider extremal horizons and develop a model-independent approach and analyze the conditions for the force to preserve or kill the effect, using the frames attached both to observers orbiting the black hole and to ones crossing the horizon. We argue that the aforementioned expectations are not confirmed. Under rather general assumptions, the BSW effect survives. For equatorial motion it is only required that in the proper frame the radial component of the force be finite, while the azimuthal one tend to zero not too slowly. If the latter condition is violated, we evaluate , which becomes indeed restricted but remains very large for small forces.
36 pages. To be published in PRD. Presentation improved, matches accepted version
References in corpus (9)
- Acceleration of particles by nonrotating charged black holes
- Collisional Penrose process near the horizon of extreme Kerr black holes
- Collision of two general geodesic particles around a Kerr black hole
- Acceleration of colliding shells around a black hole: Validity of the test particle approximation in the Banados-Silk-West process
- 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
- Transition from adiabatic inspiral to plunge into a spinning black hole
- Dirty rotating black holes: regularity conditions on stationary horizons
- Ultra-high energy collisions of nonequatorial geodesic particles near dirty black holes
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