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arXiv · 1205.1317

A novel MOND effect in isolated high-acceleration systems

Mordehai Milgrom
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Abstract

I discuss a novel MOND effect that entails a correction to the dynamics of isolated mass systems even when they are deep in the Newtonian regime: systems whose extent R< 0 is a numerical factor that depends on the interpolating function. For example, the correction to the Newtonian force between two masses, m and M, a distance L apart (L<<Rm), is Fa=2q(L/Rm)^3(mM)^2(M+m)^{-3}a0 (attractive). For generic MOND theories, which approach Newtonian dynamics quickly for accelerations beyond a0, the predicted strength of the effect in the Solar system is rather much below present testing capabilities. In MOND theories that become Newtonian only beyond k*a0, the effect is enhanced by k^2.

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Mordehai Milgrom. 2012-08-16. A novel MOND effect in isolated high-acceleration systems. https://doi.org/10.1111/j.1365-2966.2012.21719.x

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