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Loss of Mass and Stability of Galaxies in Modified Newtonian Dynamics

ASTROPHYSICAL JOURNAL, no. 2 (2007): L101-L104

Cited: 53|Views27

Abstract

The self-binding energy and stability of a galaxy in MOND-based gravity are curiously decreasing functions of its center-of-mass acceleration (of the order of 10(-12) to 10(-10) m s(-2)) toward neighboring mass concentrations. A tentative indication of this breaking of the strong equivalence principle in field galaxies is the RAVE-observe...More

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