A common Milgromian acceleration scale in nature
arXiv:1811.11754 · doi:10.1038/s41550-018-0622-x
Abstract
A central problem of contemporary physics is whether the law of gravity is non-Newtonian on galaxy scales. Rodrigues et al. argue that Milgromian gravitation, which solves the flat rotation curve problem without the need for dark matter particles, is ruled out at > 10σ significance. To a large extent, this conclusion relies on galaxies with very uncertain distances and/or nearly edge-on orientations, where dust obscuration often becomes significant. Applying appropriate quality cuts to the data leaves only a handful of outliers to the predictions of Milgromian gravitation according to the analysis of Rodrigues et al., but even these outliers can be explained with Milgromian gravitation.
arXiv commentAuthor version, published in Nature Astronomy on 13.Nov.2018 (free version: https://rdcu.be/bbuvP) as a Correspondence to the article by Rodrigues et al. http://adsabs.harvard.edu/abs/2018NatAs...2..668R; see also McGaugh et al. for a parallel Correspondence (https://www.nature.com/articles/s41550-018-0615-9); for a reply by Rodrigues et al. see https://www.nature.com/articles/s41550-018-0614-x
References in corpus (9)
- Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
- SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves
- Dipole Anisotropy in the COBE DMR First-Year Sky Maps
- The Modified Dynamics as a Vacuum Effect
- Fitting the radial acceleration relation to individual SPARC galaxies
- Galaxies appear simpler than expected
- Declining rotation curves of galaxies as a test of gravitational theory
- Absence of a fundamental acceleration scale in galaxies
- Testing Modified Newtonian Dynamics with Rotation Curves of Dwarf and Low Surface Brightness Galaxies
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- Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
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