Constraints on a fifth force from the stellar orbits around the central supermassive black hole of the Milky Way
arXiv:2604.06364 · doi:10.3390/sym18040557
Abstract
Here we investigate a possible presence of a fifth force at the Galactic Center (GC), and its potential influence on the stellar orbits around the central supermassive black hole of our Galaxy. For this purpose we simulated the stellar orbits in a Yukawa gravity model that predicts the emergence of a fifth force, and fitted them into the observed orbit of S2 star around Sgr A* at the GC. The fitting was performed using Markov chain Monte Carlo method which enabled us to constrain the parameters of Yukawa interaction describing the strength and the range of a fifth force. We studied the following cases for a fifth force range , when it is: i) about a few hundred AU (i.e. deep inside the orbit of S2 star), ii) about a thousand AU (i.e. approximately the size of S2 star orbit), and iii) several thousand AU (i.e. much larger than the size of S2 star orbit). The obtained results showed that as the range of a fifth force increases, its strength also increases and relative error decreases. The resulting fifth-force strengths in all three cases are respectively: 0.005, 0.02 and 0.15. These results are consistent with the corresponding results of both our previous studies and those of other authors, regardless of the different Yukawa-like potentials used to model a fifth force. In addition, we also studied whether the possible small discrepancies from the prediction of General Relativity for the Schwarzschild precession of S2 star could be caused by a fifth force. For this purpose we used the parameter that was recently measured in the case of S2 star by GRAVITY Collaboration in 2020. We found that the obtained estimates in all three cases are compatible, within the error intervals, with the measured value of .
18 pages, 7 tables, 4 figures. Accepted for publication in Symmetry
References in corpus (64)
- emcee: The MCMC Hammer
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Modified Gravity and Cosmology
- Extended Theories of Gravity
- Monitoring stellar orbits around the Massive Black Hole in the Galactic Center
- Measuring Distance and Properties of the Milky Way's Central Supermassive Black Hole with Stellar Orbits
- The Galactic Center Massive Black Hole and Nuclear Star Cluster
- Closest Star Seen Orbiting the Supermassive Black Hole at the Centre of the Milky Way
- Massive Gravity
- Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
- A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty
- Scalar-Tensor-Vector Gravity Theory
- Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole
- Relativistic redshift of the star S0-2 orbiting the Galactic center supermassive black hole
- An Update on Monitoring Stellar Orbits in the Galactic Center
- Bounding the mass of the graviton using gravitional-wave observations of inspiralling compact binaries
- The orbit of the star S2 around SgrA* from VLT and Keck data
- The Accelerations of Stars Orbiting the Milky Way's Central Black Hole
- Infrared-modified gravities and massive gravitons
- Data analysis recipes: Using Markov Chain Monte Carlo
- The Newtonian Limit of F(R) gravity
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- The mass distribution in the Galactic Centre from interferometric astrometry of multiple stellar orbits
- Testing General Relativity with stellar orbits around the supermassive black hole in our Galactic center
- Gravitational radiation from compact binary systems in the massive Brans-Dicke theory of gravity
- The Shortest Known Period Star Orbiting our Galaxy's Supermassive Black Hole
- Graviton Mass Bounds
- The recovery of General Relativity in massive gravity via the Vainshtein mechanism
- Dark matter vs. modifications of the gravitational inverse-square law. Results from planetary motion in the solar system
- Modelling clusters of galaxies by f(R)-gravity
- Parametrized Post-Newtonian Theory of Reference Frames, Multipolar Expansions and Equations of Motion in the N-body Problem
- Solar system vs. gravitational-wave bounds on the graviton mass
- Constraining the range of Yukawa gravity interaction from S2 star orbits
- Scalar field effects on the orbit of S2 star
- Constraining the range of Yukawa gravity interaction from S2 star orbits II: Bounds on graviton mass
- Galaxy rotation curves in -gravity
- Investigating the Binarity of S0-2: Implications for its Origins and Robustness as a Probe of the Laws of Gravity around a Supermassive Black Hole
- The Parameterised Post-Newtonian Limit of Fourth-Order Theories of Gravity
- Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
- Limits on deviations from the inverse-square law on megaparsec scales
- Constraints on the long-range properties of gravity from weak gravitational lensing
- Skewness as a test of the equivalence principle
- Search for a Variation of the Fine Structure around the Supermassive Black Hole in Our Galactic Center
- Constraining the range of Yukawa gravity interaction from S2 star orbits III: improvement expectations for graviton mass bounds
- Systematic biases on galaxy haloes parameters from Yukawa-like gravitational potentials
- Testing the Newton law at long distances
- Constraining Extended Gravity Models by S2 star orbits around the Galactic Centre
- Constraining the mass of the graviton with the planetary ephemeris INPOP
- Physical laboratory at the center of the Galaxy
- Improving constraints on the extended mass distribution in the Galactic Center with stellar orbits
- Dark energy interactions near the galactic centre
- Constraints on the range lambda of Yukawa-like modifications to the Newtonian inverse-square law of gravitation from Solar System planetary motions
- Estimating the Parameters of Extended Gravity Theories with the Schwarzschild Precession of S2 Star
- Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints
- Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
- Bounding the mass of graviton in a dynamic regime with binary pulsars
- Prospects for Constraining the Yukawa Gravity with Pulsars around Sagittarius A*
- Influence of bulk mass distribution on orbital precession of S2 star in Yukawa gravity
- A Significant Feature in the General Relativistic Time Evolution of the Redshift of Photons Coming from a Star Orbiting Sgr A*
- Estimating the parameters of Hybrid Palatini gravity model with the Schwarzschild precession of S2, S38 and S55 stars: case of bulk mass distribution
- PPN motion of the S-stars around Sgr A*
- Graviton mass and total relative density of mass Omega_tot in Universe
- Relativistic effects in orbital motion of the S-stars at the Galactic Center
- Exploring the presence of a fifth force at the Galactic Center