https://doi.org/10.1140/epjc/s10052-025-14663-3
Regular Article - Theoretical Physics
Effects of tidal charge on orbital motion in DMPR brane-world black holes
1
School of Physical Science and Technology, Southwest Jiaotong University, 610031, Chengdu, People’s Republic of China
2
School of Mathematics and Physics, University of South China, 421001, Hengyang, People’s Republic of China
a
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Received:
12
June
2025
Accepted:
21
August
2025
Published online:
1
September
2025
In this work, the orbital energy and angular momentum are calculated based on the DMPR brane-world black holes, followed by the derivation of the solution for the motion of a test particle to the second post-Newtonian order. The charge parameter Q is found to influence both the periastron advance and orbital period. In particular, its effect on perihelion precession is observed at both the first and second post-Newtonian orders, while the impact on the orbital period occurs only at the second post-Newtonian order. Furthermore, the validity of our model is confirmed by analyzing the pericenter precession of the star S2 orbiting the Galactic Center supermassive black hole Sgr A*. This nearby high-eccentricity orbit (
) provides a unique strong-gravity laboratory, yielding a constraint on the tidal charge parameter of
.
© The Author(s) 2025
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