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Observability of spherical photon orbits in near-extremal Kerr black holes

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We investigate the spherical photon orbits in near-extremal Kerr spacetimes. We show that the spherical photon orbits with impact parameters in a finite range converge on the event horizon. Furthermore,… Click to show full abstract

We investigate the spherical photon orbits in near-extremal Kerr spacetimes. We show that the spherical photon orbits with impact parameters in a finite range converge on the event horizon. Furthermore, we demonstrate that the Weyl curvature near the horizon does not generate the shear of a congruence of such light rays. Due to this property, a series of images produced by the light orbiting around a near-extremal Kerr black hole several times can be observable.

Keywords: photon orbits; spherical photon; near extremal; orbits near; extremal kerr

Journal Title: Physical Review D
Year Published: 2019

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