Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 28 min ago
PreprintCC BY 4.0HAL

Improving constraints on the Yukawa correction at the Galactic Center with multiple stellar orbits

67 more authors

60 listed; 79 in total.

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.

Related

  1. Reconciling Galactic rotation curve constraints with stellar stream modeling
    Mingyu Chang, Francois Hammer, Yanbin Yang
    arXivPreprintCC BY-NC-SA 4.0Full textGalaxiesarXiv
  2. See you again: an 80∘ NGC~5466 stellar stream and its constraints on the Galactic dark halo mass
    Di Bai, Yong Yang, Jing-Kun Zhao +2
    arXivPreprintarXiv licenceFull textGalaxiesarXiv
  3. Closed-Form of the Local Galactic Potential and Stellar Distribution Function from Gaia DR3
    Indranil Das, Adam Kamoski, Dora Demiri +3
    arXivPreprintCC BY 4.0Full textGalaxiesInstrumentation & methodsarXiv
  4. Paleodetectors for neutrino signals from diverse Galactic stellar collapses
    Mahiro Yamasaki, Ken'ichiro Nakazato
    arXivPreprintarXiv licenceFull textGalaxiesHigh-energy astrophysicsarXiv
  5. Galactic archaeology meets exoplanets: linking stellar birth radii to exoplanet demographics
    M. L. L. Dantas, J. J. García-Delgado, I. Rebollido +1
    arXivPreprintCC BY-NC-SA 4.0Full textGalaxiesPlanetary science & exoplanetsarXiv
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  -