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Acceleration of particles as universal property of rotating black holes

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arxiv 1007.3678 v2 pith:5PKDGHR3 submitted 2010-07-21 gr-qc astro-ph.HEhep-th

Oleg B. Zaslavskii This is my paper · ORCID
classification gr-qcastro-ph.HEhep-th
keywords blackholesparticlespropertyrotatingaccelerationarguecentre
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We argue that the possibility of having infinite energy in the centre of mass frame of colliding particles is a generic property of rotating black holes. We suggest a general model-independent derivation valid for "dirty" black holes. The earlier observations for the Kerr or Kerr-Newman metrics are confirmed and generalized.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Penrose and super-Penrose energy extraction from a Reissner-Nordstr\"om black hole spacetime with a cosmological constant through the BSW mechanism: Full story

    gr-qc 2024-11 conditional novelty 6.0 of 10

    For extremal charged black holes in any dimension and with any cosmological constant, a fine-tuned near-horizon particle collision can eject a particle carrying arbitrarily large, though finite, energy.

  2. Optical Landscapes and High-Energy Collisions in Hairy Horndeski Gravity

    gr-qc 2026-07 reject novelty 5.0 of 10

    For the hairy Horndeski metric, photon-sphere stability is analyzed cleanly, but the advertised Bañados-Silk-West energy divergence at Q = -2M is invalid because the critical angular momentum diverges and the collisio...

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