Exploring the presence of a fifth force at the Galactic Center

Aims. We investigate the presence of a Yukawa-like correction to Newtonian gravity at the Galactic Center, leading to a new upper limit on the intensity of such a correction. Methods. We performed a Markov chain Monte Carlo (MCMC) analysis using the astrometric and spectroscopic data of star S2 collected at the Very Large Telescope by GRAVITY, NACO, and SINFONI instruments, covering the period from 1992 to 2022. Results. The precision of the GRAVITY instrument allows us to derive the most stringent upper limit at the Galactic Center for the intensity of the Yukawa contribution (∝ αe − λr ) of | α |< 0.003 for a scale length of λ = 3 ⋅ 10 13 m (∼ 200 AU). This is an improvement on all estimates obtained in previous works by roughly one order of magnitude.

Authors

Publication Details

Journal
Astronomy and Astrophysics
Published
2025-05-22
DOI
https://doi.org/10.1051/0004-6361/202554676
Primary Topic
History and Developments in Astronomy
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Exploring the presence of a fifth force at the Galactic Center

F. Haussmann, C. Straubmeier, M. Hartl, S. Lacour et al.
Astronomy and Astrophysics
History and Developments in Astronomy
article

Exploring the presence of a fifth force at the Galactic Center

F. Haussmann, C. Straubmeier, M. Hartl, S. Lacour, G. Finger, K. Perraut, E. Wieprecht, D. C. Ribeiro, A. Drescher, S. Hippler, Pierre Léna, Jean-Philippe Berger, J. Shangguan, G. Bourdarot, A. Kaufer, R. Davies, P. T. de Zeeuw, R. Genzel, M. Horrobin, T. Ott, T. Paumard, É. Gendron, Nikhil More, Pau Amaro‐Seoane, J. Stadler, L. Tacconi, A. Eckart, Vítor Cardoso, V. Lapeyrère, G. Perrin, D. Lutz, L. Jocou, H. Feuchtgruber, Silvia Scheithauer, A. Amorim, Thomas Shimizu, S. Gillessen, P. Kervella, J.-B. Le Bouquin, X. Haubois, S. Rabien, Thomas Henning, P. García, A. Foschi, S. D. von Fellenberg, R. Abuter, N. Aimar, J. Osorno, N. M. Förster Schreiber, K. Abd El Dayem, Frédéric E. Vincent, Frank Eisenhauer, J. Woillez, L. Jochum, O. Straub, Y. Clénet, W. Brandner, F. Mang, E. Sturm, I. Urso, H. Bonnet, M. S. Bordoni
article en

Abstract

Aims. We investigate the presence of a Yukawa-like correction to Newtonian gravity at the Galactic Center, leading to a new upper limit on the intensity of such a correction. Methods. We performed a Markov chain Monte Carlo (MCMC) analysis using the astrometric and spectroscopic data of star S2 collected at the Very Large Telescope by GRAVITY, NACO, and SINFONI instruments, covering the period from 1992 to 2022. Results. The precision of the GRAVITY instrument allows us to derive the most stringent upper limit at the Galactic Center for the intensity of the Yukawa contribution (∝ αe − λr ) of | α |< 0.003 for a scale length of λ = 3 ⋅ 10 13 m (∼ 200 AU). This is an improvement on all estimates obtained in previous works by roughly one order of magnitude.

Astronomy and AstrophysicsVol. 698
National Science Foundation, European Commission, Deutsche Forschungsgemeinschaft, National Natural Science Foundation of China, Bundesministerium für Bildung und Forschung, Max-Planck-Gesellschaft, European Southern Observatory, Centre National de la Recherche Scientifique, Centre National pour la Recherche Scientifique et Technique, Observatoire de Paris, Université de Recherche Paris Sciences et Lettres, European Research Council, Fundação para a Ciência e a Tecnologia
Openalex Percentile: Top 92%
History and Developments in Astronomy
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.