Baryonic matter alone, with gravitational self-interaction treated as a 1/r force in disks, reproduces the observed radial acceleration relation and yields an acceleration scale matching MOND.
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Significance of Gravitational Nonlinearities on the Dynamics of Disk Galaxies
Baryonic matter alone, with gravitational self-interaction treated as a 1/r force in disks, reproduces the observed radial acceleration relation and yields an acceleration scale matching MOND.