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Chaos around the superposition of a black-hole and a thin disk

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arxiv gr-qc/9906028 v1 pith:HRTH7H3L submitted 1999-06-07 gr-qc

Alberto Saa , Roberto Venegeroles This is my paper · ORCID
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keywords diskaroundblack-holelimitsrelativisticsuperpositionthinwere
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Motivated by the strong astronomical evidences supporting that huge black-holes might inhabit the center of many active galaxies, we have studied the integrability of oblique orbits of test particles around the exact superposition of a black-hole and a thin disk. We have considered the relativistic and the Newtonian limits. Exhaustive numerical analyses were performed, and bounded zones of chaotic behavior were found for both limits. An intrinsic relativistic gravitational effect is detected: the chaoticity of trajectories that do not cross the disk.

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Cited by 1 Pith paper

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  1. Chaotic orbital dynamics of pulsating stars around black holes surrounded by dark matter halos

    gr-qc 2024-12 conditional novelty 6.0 of 10

    Spherically symmetric pulsations trigger homoclinic chaos in orbits around black holes enclosed by dark matter halos, unlike the vacuum Schwarzschild case.

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