The Radial Acceleration Relation in Rotationally Supported Galaxies

Abstract

We report a correlation between the radial acceleration traced by rotation curves and that predicted by the observed distribution of baryons. The same relation is followed by 2693 points in 153 galaxies with very different morphologies, masses, sizes, and gas fractions. The correlation persists even when dark matter dominates. Consequently, the dark matter contribution is fully specified by that of the baryons. The observed scatter is small and largely dominated by observational uncertainties. This radial acceleration relation is tantamount to a natural law for rotating galaxies.

arXiv comment6 pages, 3 figures. Accepted for publication in Physical Review Letters

References in corpus (36)

• A Universal Density Profile from Hierarchical Clustering
• Stellar mass-to-light ratios and the Tully-Fisher relation
• The Baryonic Tully-Fisher Relation
• The Core-Cusp Problem
• The Ursa Major Cluster of Galaxies. V ; HI Rotation Curve Shapes and the Tully-Fisher Relations
• The dark and baryonic matter content of low surface brightness disk galaxies
• Testing the Dark Matter Hypothesis with Low Surface Brightness Galaxies and Other Evidence
• Galaxy And Mass Assembly (GAMA): mass-size relations of z$<$0.1 galaxies subdivided by Sérsic index, colour and morphology
• The small scatter of the baryonic Tully-Fisher relation
• Dwarf Galaxy Rotation Curves and the Core Problem of Dark Matter Halos
• Reconstructing the stellar mass distributions of galaxies using S4G IRAC 3.6 and 4.5 micron images: II. The conversion from light to mass
• Color--Mass-to-Light Ratio Relations for Disk Galaxies
• The Mass Discrepancy-Acceleration Relation: Disk Mass and the Dark Matter Distribution
• A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
• The DiskMass Survey. VII. The distribution of luminous and dark matter in spiral galaxies
• The Tully-Fisher relation for low surface brightness galaxies - implications for galaxy evolution
• A New Approach to Systematic Uncertainties and Self-Consistency in Helium Abundance Determinations
• Weighing Galaxy Disks with the Baryonic Tully-Fisher Relation
• Milky Way Mass Models and MOND
• A Tale of Two Paradigms: the Mutual Incommensurability of LCDM and MOND
• The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies
• A Study in Blue: The Baryon Content of Isolated Low Mass Galaxies
• Gravitational polarization and the phenomenology of MOND
• Does low surface brightness mean low surface density?
• The mass discrepancy acceleration relation in a $\Lambda$CDM context
• An Alternative to Particle Dark Matter
• Missing dark matter in dwarf galaxies?
• The Balance of Dark and Luminous Mass in Rotating Galaxies
• The HI Tully-Fisher Relation of Early-Type Galaxies
• Stellar Populations and the Star Formation Histories of LSB Galaxies: III. Stellar Population Models
• A scaling-relation for disc galaxies: circular-velocity gradient versus central surface brightness
• Linear relation between HI circular velocity and stellar velocity dispersion in early-type galaxies, and slope of the density profiles
• Dark Fluid: Towards a unification of empirical theories of galaxy rotation, Inflation and Dark Energy
• Modified Newtonian Dynamics, an Introductory Review
• Stellar Populations and the Star Formation Histories of LSB Galaxies: IV Spitzer Surface Photometry of LSB Galaxies
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions

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