Citation: Della Monica, R.; de
Martino, I.; de Laurentis, M.
Constraining MOdified Gravity with
with the S2 Star. Universe 2022, 8, 137.
https://doi.org/10.3390/
universe8020137
Academic Editors: Mariusz P.
D˛ abrowski, Adam Balcerzak and
Vincenzo Salzano
Received: 24 January 2022
Accepted: 16 February 2022
Published: 21 February 2022
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universe
Communication
Constraining MOdified Gravity with the S2 Star
Riccardo Della Monica
1,
* , Ivan de Martino
1
and Mariafelicia de Laurentis
2,3
1
Departamento de Fisica Fundamental, Universidad de Salamanca, P. de la Merced, 37008 Salamanca, Spain;
ivan.demartino@usal.es
2
Dipartimento di Fisica, Universitá di Napoli “Federico II”, Complesso Universitario di Monte S. Angelo,
Edificio G, Via Cinthia, I-80126 Napoli, Italy; mariafelicia.delaurentis@unina.it
3
INFN Sezione di Napoli, Complesso Universitario di Monte S. Angelo, Edificio G, Via Cinthia,
I-80126 Napoli, Italy
* Correspondence: rdellamonica@usal.es
Abstract: We have used publicly available kinematic data for the S2 star to constrain the parameter
space of MOdified Gravity. Integrating geodesics and using a Markov Chain Monte Carlo algorithm,
we have provided the first constraint on the scales of the Galactic Centre for the parameter α of the
theory, which represents the fractional increment of the gravitational constant G with respect to its
Newtonian value. Namely, α 0.662 at 99.7% confidence level (where α = 0 reduces the theory to
General Relativity).
Keywords: alternative gravity; galactic centre; black holes
1. Introduction
Scalar-Tensor-Vector Gravity (STVG), also referred to in the literature as MOdified
Gravity (MOG), is a theory of gravity firstly proposed in [1] as an alternative to Einstein’s
theory of General Relativity (GR). It introduces extra fields in the description of the gravita-
tional interaction, allowing for correct predictions on galactic and extragalactic scales [2–6],
without resorting to dark matter [7]. The gravitational action in MOG presents additional
terms along the classical Hilbert–Einstein action, depending on the metric tensor g
αβ
of
spacetime. More specifically, a massive vector field ϕ
α
is introduced and its mass, μ, is
treated as a scalar field. Furthermore, Newton’s gravitational constant G
N
is also elevated
to a scalar field G.
The motion of test particles in MOG is affected by the presence of the vector field ϕ
α
which acts as a fifth force, whose repulsive character counteracts the increased attraction due
to the scalar field nature of G. The fractional increment of G, with respect to its Newtonian
value, G
N
, is given by a new parameter of the theory, α =(G − G
N
)/G
N
. A distinctive
feature in the motion of test massive bodies in MOG is that Keplerian orbits in a central
potential are characterized by an increased value of the rate of orbital precession [8,9]. This
is given by:
Δω
MOG
= Δω
GR
1 +
5
6
α
, (1)
where Δω
GR
is the usual expression of the periastron advance in GR,
Δω
GR
=
6πG
N
M
ac
2
(1 − e
2
)
, (2)
related to semi-major axis, a, and eccentricity, e, of the orbiting body.
Here, we will summarize the extended work carried out in [8], where we used publicly
available data for the S2 star from [10], along with the measurement of its orbital precession
from [11] to constrain the parameter space of MOG.
Universe 2022, 8, 137. https://doi.org/10.3390/universe8020137 https://www.mdpi.com/journal/universe