Document Type
Article
Publication Date
11-21-2022
Abstract
The strong equivalence principle is violated by gravity theories of Milgromian dynamics [modified Newtonian dynamics (MOND)] through the action of the external field effect. We test two different Lagrangian theories Aquadratic-Lagrangian (AQUAL) and quasilinear MOND (QUMOND) based on their numerical solutions of the external field effect, by comparing two independent estimates of the mean external field strength of the nearby universe: a theory-deduced value from fitting the outer rotation curves of 114 galaxies and an empirical value from the large-scale distribution of cosmic baryons. The AQUAL-deduced external field strength from rotation curves agrees with that from the large-scale cosmic environment, while QUMOND-deduced value is somewhat higher. This suggests that AQUAL is likely to be preferred over QUMOND as an effective nonrelativistic limit of a potential relativistic modified gravity theory.
Keywords
alternative gravity theories, dark matter, gravitation
Publication Title
Physical Review D
Grant
211046
Rights
© 2022 American Physical Society. Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Recommended Citation
Chae, Kyu-Hyun and Lelli, Federico and Desmond, Harry and McGaugh, Stacy S. and Schombert, James M. Testing modified gravity theories with numerical solutions of the external field effect in rotationally supported galaxies. Phys. Rev. D, vol106, issue10, 2022. doi: 10.1103/PhysRevD.106.103025
Manuscript Version
Final Publisher Version