Improving constraints on the Yukawa correction at the Galactic Center with multiple stellar orbits
Abstract
We investigate the presence of a Yukawa-like correction (∝ αe− r/λ) to Newtonian gravity at the Galactic Center, using a multi-star fitting code, including the newly discovered star S$301$, to improve the constraints obtained using S$2$ orbit alone. We perform a Markov Chain Monte Carlo analysis using the astrometric and spectroscopic data of stars S$2$, S$55$, S$29$, S$38$ and S$301$ collected by GRAVITY, GRAVITY+, NACO and SINFONI instruments, covering the period from $1992$ to $2025$. Compared to GRAVITY Collaboration 2025 (Paper I), in which only S$2$ was fitted, the tightest bound on the Yukawa coupling is again reached at λ= 3·1013 m (∼ 200 AU), where we find |α| < 6 ·10−4, an improvement of roughly a factor five. The addition of S$301$ extends the constraint to short ranges that were inaccessible to S$2$, yielding |α| < 0.004 at λ=1012 m and |α| < 0.006 at λ=5· 1011 m, while S$29$, with its larger apoapsis, gives |α| < 0.1 at λ∼ 2·1015 m. The latter two represent the tightest limits at these scale lengths on a Yukawa correction obtained to date around a supermassive black hole.
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BibTeX
@misc{foschi2026improving,
title = {{Improving constraints on the Yukawa correction at the Galactic Center with multiple stellar orbits}},
author = {A Foschi and K Abd El Dayem and N Aimar and A Berdeu and J.-P Berger and G Bourdarot and W Brandner and Y Cao and C Correia and S. Cueves Cardona and R Davies and D Defrère and F Delplancke-Ströbele and A Drescher and F Eisenhauer and L. Esteras Otal and M Fabricius and H Feuchtgruber and S Flesch and N.M. Förster Schreiber and Q Fournier and P Garcia and R. Garcia Lopez and R Genzel and S Gillessen and F Gonté and X Haubois and S.F Hönig and M Houllé and S Joharle and J Kammerer and A Kaufer and P Kervella and L Kreidberg and L Labadie and S Lacour and O Lai and R Laugier and J.-B Le Bouquin and J Leftley and R Li and B Lopez and D Lutz and F Mang and A Mérand and F Millour and M Montargès and N Morujão and H Nowacki and M Nowak and J Osorno and T Ott and S Pappert and C Paladini and T Paumard and K Perraut and G Perrin and R Petrov and N Pourré and S Rabien},
howpublished = {HAL},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.07693},
eprint = {2609.07693},
archivePrefix = {arXiv},
url = {https://hal.science/hal-05761038v1},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Improving constraints on the Yukawa correction at the Galactic Center with multiple stellar orbits
AU - A Foschi
AU - K Abd El Dayem
AU - N Aimar
AU - A Berdeu
AU - J.-P Berger
AU - G Bourdarot
AU - W Brandner
AU - Y Cao
AU - C Correia
AU - S. Cueves Cardona
AU - R Davies
AU - D Defrère
AU - F Delplancke-Ströbele
AU - A Drescher
AU - F Eisenhauer
AU - L. Esteras Otal
AU - M Fabricius
AU - H Feuchtgruber
AU - S Flesch
AU - N.M. Förster Schreiber
AU - Q Fournier
AU - P Garcia
AU - R. Garcia Lopez
AU - R Genzel
AU - S Gillessen
AU - F Gonté
AU - X Haubois
AU - S.F Hönig
AU - M Houllé
AU - S Joharle
AU - J Kammerer
AU - A Kaufer
AU - P Kervella
AU - L Kreidberg
AU - L Labadie
AU - S Lacour
AU - O Lai
AU - R Laugier
AU - J.-B Le Bouquin
AU - J Leftley
AU - R Li
AU - B Lopez
AU - D Lutz
AU - F Mang
AU - A Mérand
AU - F Millour
AU - M Montargès
AU - N Morujão
AU - H Nowacki
AU - M Nowak
AU - J Osorno
AU - T Ott
AU - S Pappert
AU - C Paladini
AU - T Paumard
AU - K Perraut
AU - G Perrin
AU - R Petrov
AU - N Pourré
AU - S Rabien
PY - 2026
DA - 2026/09/09
PB - HAL
DO - 10.48550/arxiv.2609.07693
UR - https://hal.science/hal-05761038v1
AB - We investigate the presence of a Yukawa-like correction (∝ αe^− r/λ) to Newtonian gravity at the Galactic Center, using a multi-star fitting code, including the newly discovered star S$301$, to improve the constraints obtained using S$2$ orbit alone. We perform a Markov Chain Monte Carlo analysis using the astrometric and spectroscopic data of stars S$2$, S$55$, S$29$, S$38$ and S$301$ collected by GRAVITY, GRAVITY^+, NACO and SINFONI instruments, covering the period from $1992$ to $2025$. Compared to GRAVITY Collaboration 2025 (Paper I), in which only S$2$ was fitted, the tightest bound on the Yukawa coupling is again reached at λ= 3·10^13 m (∼ 200 AU), where we find |α| < 6 ·10^−4, an improvement of roughly a factor five. The addition of S$301$ extends the constraint to short ranges that were inaccessible to S$2$, yielding |α| < 0.004 at λ=10^12 m and |α| < 0.006 at λ=5· 10^11 m, while S$29$, with its larger apoapsis, gives |α| < 0.1 at λ∼ 2·10^15 m. The latter two represent the tightest limits at these scale lengths on a Yukawa correction obtained to date around a supermassive black hole.
ER -