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Rapidly rotating Kerr black holes can accelerate particles to arbitrarily high energy if the angular momentum of the particle is fine-tuned to some critical value.
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O. B. Zaslavskii, “Acceleration of particles by black holes: kinematic explanation,” Phys. Rev. D 84
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2011
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2011
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2011
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2011
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2011
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2011
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2011
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S. Aretakis, “Stability and Instability of Extreme Reissner-Nordstróm Black Hole Spacetimes for Linear Scalar Perturbations II,” Ann. Henri Poincaré 12
2011
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2012
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Z. Stuchlík and J. Schee, “Observational phenomena related to primordial Kerr superspinars,” Class. Quant. Grav. 29
2012
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S. T. McWilliams, “Black Holes are neither Particle Accelerators nor Dark Matter Probes” Phys. Rev. Lett. 110
2013
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2013
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2013
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S. Aretakis, “Nonlinear instability of scalar fields on extremal black holes,” Phys. Rev. D 87
2013
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2013
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K. Murata, “Instability of higher dimensional extreme black holes,” Class. Quant. Grav. 30
2013
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2013
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2013
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2014
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J. Gariel, N. O. Santos and J. Silk, “Unbound geodesics from the ergosphere and potential observability of debris from ultrahigh energy particle collisions” Phys. Rev. D 90
2014
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2014
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