{ "id": "2112.00026", "version": "v2", "published": "2021-11-30T19:00:03.000Z", "updated": "2022-09-20T05:27:21.000Z", "title": "The phenomenology of the external field effect in cold dark matter models", "authors": [ "Aseem Paranjape", "Ravi K. Sheth" ], "comment": "11 pages, 6 figures; v2: minor changes and added discussion, accepted in MNRAS", "categories": [ "astro-ph.CO", "astro-ph.GA" ], "abstract": "In general relativity (GR), the internal dynamics of a self-gravitating system under free-fall in an external gravitational field should not depend on the external field strength. Recent work has claimed a statistical detection of an `external field effect' (EFE) using galaxy rotation curve data. We show that large uncertainties in rotation curve analyses and inaccuracies in published simulation-based external field estimates compromise the significance of the claimed EFE detection. We further show analytically that a qualitatively similar statistical signal is, in fact, expected in a $\\Lambda$-cold dark matter ($\\Lambda$CDM) universe without any violation of the strong equivalence principle. Rather, such a signal arises simply because of the inherent correlations between galaxy clustering strength and intrinsic galaxy properties. We explicitly demonstrate the effect in a baryonified mock catalog of a $\\Lambda$CDM universe. Although the detection of an EFE-like signal is not, by itself, evidence for physics beyond GR, our work shows that the $\\textit{sign}$ of the EFE-like correlation between the external field strength and the shape of the radial acceleration relation can be used to probe new physics: e.g., in MOND, the predicted sign is opposite to that in our $\\Lambda$CDM mocks.", "revisions": [ { "version": "v2", "updated": "2022-09-20T05:27:21.000Z" } ], "analyses": { "keywords": [ "cold dark matter models", "external field effect", "external field estimates compromise", "simulation-based external field estimates", "external field strength" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }