Abstract
We consider a head-on collision of two massive particles that move in the equatorial plane of an extremal Kerr black hole, which results in the production of two massless particles. Focusing on a typical case, where both of the colliding particles have zero angular momenta, we show that a massless particle produced in such a collision can escape to infinity with arbitrarily large energy in the near-horizon limit of the collision point. Furthermore, if we assume that the emission of the produced massless particles is isotropic in the center-of-mass frame but confined to the equatorial plane, the escape probability of the produced massless particle approaches , and almost all escaping massless particles have arbitrarily large energy at infinity and an impact parameter approaching , where is the mass of the black hole.
- Received 14 October 2016
DOI:https://doi.org/10.1103/PhysRevD.95.124019
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