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On the collisions between particles in the vicinity of rotating black holes

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arxiv 1004.0913 v2 pith:ZYRD3NFS submitted 2010-04-06 gr-qc

classification gr-qc
keywords blackparticlesenergyholesescapingholelargerotating
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Scattering of particles in the gravitational field of rotating black holes is considered. It is shown that scattering energy of particles in the centre of mass system can obtain very large values not only for extremal black holes but also for nonextremal ones. Extraction of energy after the collision is investigated. It is shown that due to the Penrose process the energy of the particle escaping the hole at infinity can be large. Contradictions in the problem of getting high energetic particles escaping the black hole are resolved.

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  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.

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