Emergent Flux from Particle Collisions Near a Kerr Black Hole

Details Emergent Flux from Particle Collisions Near a Kerr Black Hole Emergent Flux from Particle Collisions Near a Kerr Black Hole

2010-10-13

arxiv.org/abs/1010.2724v1

Phys.Rev.D83:023004,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

10 Pages, 5 Figures

Scientific paper

10.1103/PhysRevD.83.023004

The escape fraction at infinity is evaluated for massless particles produced in collisions of weakly interacting particles accreted into a density spike near the particle horizon of an extremal Kerr black hole, for the case of equatorial orbits. We compare with the Schwarzschild case, and argue that in the case of extremal black holes, redshifted signatures can be produced that could potentially explore the physics of particle collisions at centre of mass energies that extend beyond those of any feasible terrestrial accelerator.

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