In this paper we provide observational evidence for the existence of the EFE (or a phenomenon akin to it) predicted by MOND modified gravity (Bekenstein & Milgrom 1984). We use accurate rotation curves and mass models from the SPARC database (Lelli et al. 2016) and detect the EFE in three separate ways:

  • 1.
    The EFE is individually detected in “golden” galaxies subjected to exceptionally strong external gravitational fields. The detection is highly significant (11σ in NGC 5055 and 8σ in NGC 5033) and the best-fit values of the external gravitational fields are fully consistent with the independent estimates from the large-scale distribution of mass at the galaxies’ location. Conversely, the EFE is not detected in control galaxies residing in the weakest external gravitational fields, as expected.
  • 2.
    The EFE is statistically detected at more than 4σ through a blind test using 153 SPARC galaxies. The mean value of the external gravitational field among the SPARC galaxies is again consistent with the independent estimate from the average distribution of mass in the nearby universe.
  • 3.
    The EFE also manifests as a small (≳0.05 dex), downward deviation from the empirical RAR occurring around 0.1g. This behavior is not predicted by any of the existing galaxy formation models in ΛCDM that were proposed to “naturally” reproduce the RAR. In contrast, this downward deviation is predicted by the MOND modified gravity at the right acceleration scale.

Our results suggest a breakdown of the SEP: the internal dynamics of a gravitational system in freefall is affected by a uniform external gravitational field. This sheds new light on the dark-matter problem and paves the way for relativistic theories of modified gravity in the weak-field regime of gravity g ≲ 10−10 m s−2.

We thank the organizers of the conference Bonn-Gravity 2019 (Pavel Kroupa and Indranil Banik) where several of these issues were brought to light. We thank Andrey Kravtsov for providing a code to calculate tidal radii of ΛCDM halos.

This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. NRF-2019R1F1A1062477). H.D. is supported by St John’s college, Oxford, and acknowledges financial support from ERC grant No. 693024 and the Beecroft Trust. The Work of S.S.M. is supported in part by NASA ADAP 80NSSC19k0570 and NSF PHY-1911909.

This is taken from a long paper. Read the rest here: iopscience.iop.org

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