On the Evidence for Violation of the Equivalence Principle in Disk Galaxies
Corey Sargent, William Clark, Antonia Seifert, Alicia Mand, Emerson Rogers, Adam Lane, Alexandre Deur, Balša Terzić
TL;DR
The paper investigates whether external-field effects claimed in disk galaxies signal a violation of the equivalence principle. It introduces a General Relativity self-interaction (GR-SI) framework in which $g_{SI}(r) = g_{3D}(r) + g_{2D}(r)$ with $g_{2D}(r) = sqrt(G alpha) sqrt(M_D(r)) / r$ and uses morphology and environment proxies to connect to observed dynamics. Through ~40,000 simulated galaxies and an MCMC-style analysis, it shows that morphology–environment correlations can reproduce the radial-acceleration relation and suppress apparent EFE, challenging the interpretation of ChaE et al.'s claims. The results indicate that current observational data do not decisively support an EFE and highlight convergence issues in prior MCMC analyses, underscoring the need for more robust tests of GR self-interaction versus MOND-like behavior.
Abstract
We examine the claimed observations of a gravitational external field effect (EFE) reported in Chae et al. We show that observations suggestive of the EFE can be interpreted without violating Einstein's equivalence principle, namely from known correlations between morphology, environment and dynamics of galaxies. While Chae et al's analysis provides a valuable attempt at a clear test of Modified Newtonian Dynamics, an evidently important topic, a re-analysis of the observational data does not permit us to confidently assess the presence of an EFE or to distinguish this interpretation from that proposed in this article.
