Response to: Comment on "Orbital precession of the S2 star in scalar-tensor-vector gravity"
arXiv:2302.12296 · doi:10.1093/mnras/stad579
Abstract
The explicit derivation for the orbital precession of the S2 star in the Galactic Center in the Scalar-Tensor-Vector Gravity is discussed and compared with previous research. The two different predictions are validated by numerically integrating the geodesic equations for a test particle.
4 pages, 2 figures, 1 appendix. Accepted for publication in MNRAS
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