Response to: Comment on "Orbital precession of the S2 star in scalar-tensor-vector gravity"

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

References in corpus (8)

• Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole
• An Update on Monitoring Stellar Orbits in the Galactic Center
• Black Holes in Modified Gravity (MOG)
• The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter
• Rotational Velocity Curves in the Milky Way as a Test of Modified Gravity
• Fundamental parameter-free solutions in Modified Gravity
• Orbital precession of the S2 star in Scalar-Tensor-Vector-Gravity
• Giant low-surface-brightness dwarf galaxy as a test bench for MOdified Gravity

Cited by in corpus (6)

• The Galactic Center as a laboratory for theories of gravity and dark matter
• Gravitational synchrotron radiation and Penrose process in STVG theory
• Testing space-time geometries and theories of gravity at the Galactic Center with pulsar's time delay
• Constraints on metric-affine gravity black holes from the stellar motion at the Galactic Center
• Dynamics of Dwarf Galaxies in Scalar-Tensor-Vector-Gravity
• Detecting Lorentz-violation induced by a tensor field with S-star's motion around Sgr A*