Circular motion of test particles, trajectories and QPOs around the non-rotating black hole in the background of the Symmergent gravity

We explore the circular motion of test particles around the non-rotating black hole in the background of the Symmergent gravity, focusing on how the parameters of the underlying model influence particle motion. The black hole is fully characterized by four parameters, namely, the mass M of the black...

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Bibliographic Details
Published in:PHYSICS OF THE DARK UNIVERSE 2025-02, Vol.47, p.101806, Article 101806
Main Authors: Maurya, S.K., Mustafa, G., Ditta, Allah, Abd-Elmonem, Assmaa, Alhubieshi, Neissrien, Caliskan, Aylin, Güdekli, Ertan
Format: Article
Language:English
Subjects:
Black holes
Circular orbits
Particle motion
Quasi-periodic oscillations
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Summary:We explore the circular motion of test particles around the non-rotating black hole in the background of the Symmergent gravity, focusing on how the parameters of the underlying model influence particle motion. The black hole is fully characterized by four parameters, namely, the mass M of the black hole, the charge q of the black hole, and two parameters η and α, with η>1 (η
ISSN:2212-6864
2212-6864
DOI:10.1016/j.dark.2025.101806