The radial acceleration relation and its emergent nature
arXiv:2005.12384 · doi:10.1017/S1743921320001684
Abstract
We review some of our recent results about the Radial Acceleration Relation (RAR) and its interpretation as either a fundamental or an emergent law. The former interpretation is in agreement with a class of modified gravity theories that dismiss the need for dark matter in galaxies (MOND in particular). Our most recent analysis, which includes refinements on the priors and the Bayesian test for compatibility between the posteriors, confirms that the hypothesis of a fundamental RAR is rejected at more than 5 from the very same data that was used to infer the RAR.
2 pages, 1 figure. To appear in the Proceedings IAU Symposium No. 359, 2020. Galaxy evolution and feedback across different environments (Galfeed)
References in corpus (7)
- SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- Fitting the radial acceleration relation to individual SPARC galaxies
- Absence of a fundamental acceleration scale in galaxies
- The Intrinsic Scatter of the Radial Acceleration Relation
- Reply to "Presence of a fundamental acceleration scale in galaxies" and "A common Milgromian acceleration scale in nature"
- Reply to: Overconfidence in Bayesian analyses of galaxy rotation curves