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Inspirals from the innermost stable circular orbit of Kerr black holes: Exact solutions and universal radial flow

Published 8 Sep 2022 in gr-qc and astro-ph.HE | (2209.03579v1)

Abstract: We present exact solutions of test particle orbits spiralling inward from the innermost stable circular orbit (ISCO) of a Kerr black hole. Our results are valid for any allowed value of the angular momentum $a$-parameter of the Kerr metric. These solutions are of considerable physical interest. In particular, the radial 4-velocity of these orbits is both remarkably simple and, with the radial coordinate scaled by its ISCO value, universal in form, otherwise completely independent of the black hole spin.

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