Free motion around black holes with discs or rings: between integrability and chaos - II
O. Semer\'ak, P. Sukov\'a

TL;DR
This paper investigates the complex dynamics of test particles around black holes with surrounding discs or rings, revealing varying degrees of chaos and applying novel recurrence analysis methods to classify orbital behaviors.
Contribution
It extends previous work by comparing detailed orbit classifications using power spectra and recurrence methods, enhancing understanding of chaos in black hole environments.
Findings
Orbits exhibit a wide range of chaoticity levels.
Recurrence methods effectively classify orbital behaviors.
Power spectra shape correlates with orbit dynamics.
Abstract
We continue the study of time-like geodesic dynamics in exact static, axially and reflection symmetric space-times describing the fields of a Schwarzschild black hole surrounded by thin discs or rings. In the previous paper, the rise (and decline) of geodesic chaos with ring/disc mass and position and with test particle energy was revealed on Poincar\'e sections, on time series of position or velocity and their power spectra, and on time evolution of the orbital `latitudinal action'. In agreement with the KAM theory of nearly integrable dynamical systems and with the results observed in similar gravitational systems in the literature, we found orbits of very different degrees of chaoticity in the phase space of perturbed fields. Here we compare selected orbits in more detail and try to classify them according to the characteristics of the corresponding phase-variable time series, mainly…
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