Response to: Comment on ‘Orbital precession of the S2 star in scalar–tensor–vector gravity’

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 Centre 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....

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society Vol. 521; no. 1; pp. 474 - 477
Main Authors: Della Monica, Riccardo, de Martino, Ivan, de Laurentis, Mariafelicia
Format: Journal Article
Language:English
Published: Oxford University Press 02-03-2023
Subjects:
stars: black hole
stars: kinematics and dynamics
gravitation
Galaxy: centre
dark matter
Online Access:Get full text
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Summary:ABSTRACT The explicit derivation for the orbital precession of the S2 star in the Galactic Centre 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.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stad579