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Exact solutions and approximations of MOND fields of disc galaxies

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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1995-09-15 and is currently open access. It has received 112 citations till now. The article focuses on the topics: Stellar dynamics & Disc galaxy.

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Modified Newtonian dynamics as an alternative to dark matter

TL;DR: Modified Newtonian dynamics (MOND) is an empirically motivated modification of Newtonian gravity or inertia suggested by Milgrom as an alternative to cosmic dark matter as mentioned in this paper.
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Modified Newtonian Dynamics (MOND):Observational Phenomenology and Relativistic Extensions

TL;DR: It is shown that many of these puzzling observations are predicted by one single relation — Milgrom’s law — involving an acceleration constant a0 on the order of the square-root of the cosmological constant in natural units.
Journal ArticleDOI

Modified Newtonian dynamics in the Milky Way

TL;DR: In this paper, the authors investigated the predictions of the modified Newtonian dynamics (MOND) formula for the Galaxy given the measured baryon distribution and obtained satisfying fits to the observationally determined terminal-velocity curve.
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One Law To Rule Them All: The Radial Acceleration Relation of Galaxies

TL;DR: In this paper, the authors studied the radial acceleration relation between baryons and dark matter in 240 galaxies with spatially resolved kinematic data and found that the relationship coincides with the 1:1 line (no dark matter) at high accelerations but systematically deviates from unity below a critical scale of ~10^-10 m/s^2.
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The modified Newtonian dynamics-MOND-and its implications for new physics

TL;DR: In this article, a relativistic version of the modified Newtonian dynamics (MOND) has been proposed to interpret observations without appeal to invisible dark matter. But the MOND paradigm could not address gravitational lensing or cosmology.
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