The MOND limit from space-time scale invariance
Mordehai Milgrom

TL;DR
This paper shows that the MOND limit can be derived from space-time scale invariance principles, linking deep-MOND phenomena to fundamental symmetry and cosmological geometry, offering a new perspective on modified gravity theories.
Contribution
It proposes that the MOND limit follows from space-time scale invariance, replacing the low-acceleration criterion, and explores its implications for cosmology and dark matter interpretations.
Findings
Deep-MOND results follow from scale invariance symmetry.
Asymptotic flat rotation curves result from scaling properties.
MOND may be connected to de Sitter universe geometry.
Abstract
The MOND limit is shown to follow from a requirement of space-time scale invariance of the equations of motion for nonrelativistic, purely gravitational systems; i.e., invariance of the equations of motion under (t,r) goes to (qt,qr), in the limit a0 goes to infinity. It is suggested that this should replace the definition of the MOND limit based on the low-acceleration behavior of a Newtonian-MOND interpolating function. In this way, the salient, deep-MOND results--asymptotically flat rotation curves, the mass-rotational-speed relation (baryonic Tully-Fisher relation), the Faber-Jackson relation, etc.--follow from a symmetry principle. For example, asymptotic flatness of rotation curves reflects the fact that radii change under scaling, while velocities do not. I then comment on the interpretation of the deep-MOND limit as one of "zero mass": Rest masses, whose presence obstructs…
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