Near horizon geometry of extremal black holes and Banados-Silk-West effect
arXiv:1301.1159 · doi:10.1103/PhysRevD.88.027505
Abstract
Recently, Banados, Silk and West analyzed a collision of two particles near the horizon of the extremal Kerr black hole and demonstrated that the energy in the center-of-mass frame can be arbitrarily large provided the angular momentum of one of the colliding particles takes a special value. As is known, the vicinity of the extremal Kerr black hole horizon can be viewed as a complete vacuum spacetime in its own right. In this work, we consider a collision of two neutral particles within the context of the near horizon extremal Kerr geometry and demonstrate that the energy in the center-of-mass frame is finite for any admissible value of the particle parameters. An explanation of why the two approaches disagree on the Banados-Silk-West effect is given.
V5:10 pages, major revision, title changed; the version published in PRD
References in corpus (10)
- CFT Duals for Extreme Black Holes
- Charged Spinning Black Holes as Particle Accelerators
- Collisional Penrose process near the horizon of extreme Kerr black holes
- Emergent Flux from Particle Collisions Near a Kerr Black Hole
- Acceleration of particles by black holes -- general explanation
- Acceleration of colliding shells around a black hole: Validity of the test particle approximation in the Banados-Silk-West process
- Particle dynamics near extreme Kerr throat and supersymmetry
- Black Holes are neither Particle Accelerators nor Dark Matter Probes
- Near horizon black holes in diverse dimensions and integrable models
- Acceleration of particles by acceleration horizons
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