By Prerna Rana and Arun Mangalam at

Tata Institute of Fundamental Research

and Indian Institute of Astrophysics

We derive the conditions for a non-equatorial eccentric bound orbit to exist around a Kerr black hole in two-parameter spaces: the energy, angular momentum of the test particle, spin of the black hole, and Carter's constant space (\(E\), \(L\), \(a\), \(Q\)), and eccentricity, inverse-latus rectum space (\(e\), \(\mu\), \(a\), \(Q\)).... Show more

July 12, 2022

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Bound orbit domains in the phase space of the Kerr geometry

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