The properties and predictions of quasi-periodic oscillations around a black hole in nonlocal gravity

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This research aims to examine the dynamics of massive test particles around black holes in nonlocal gravity and their effects on quasi-periodic oscillations (QPOs).
Analyzed the dynamics of test particles around a static black hole in the context of nonlocal gravity.
Constrained the nonlocal parameter and evaluated its effects on effective potential, energy, and angular momentum of orbits.
Found that increasing the nonlocal parameter substantially reduces the energy and angular momentum of circular orbits, decreasing the ISCO radius.
Observed that the radiative efficiency increases up to approximately 8.9%.
Demonstrated that the resonance condition affects the resonant radius and the range of predicted QPO frequencies.

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Investigates properties of quasi-periodic oscillations in black holes, suggesting implications for gravity theories.

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Sui et al. (2026) studied this question.

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