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Bound orbit domains in the phase space of the Kerr geometry

By Prerna Rana and Arun Mangalam at
LogoTata Institute of Fundamental Research
and
LogoIndian 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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