Response to: Comment on ‘Orbital precession of the S2 star in scalar–tensor–vector gravity’
Riccardo Della MonicaDepartamento de Fisica Fundamental, Universidad de Salamanca , P. de la Merced, Salamanca, ES 37008, SpainIvan De MartinoDepartamento de Fisica Fundamental, Universidad de Salamanca , P. de la Merced, Salamanca, ES 37008, SpainMariafelicia De LaurentisDipartimento di Fisica, Universitá di Napoli ‘Federico II’, Compl. Univ. di Monte S. Angelo , Edificio G, Via Cinthia, I-80126 Napoli, Italy
2023en
ABI
Annotatsiya
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.
Hali tarjima qilinmagan
Identifikatorlar
Iqtiboslar va manbalar
3 ta iqtibos0 ta foydalanilgan manba