
arXiv: 1604.06378
handle: 11368/2890577
MOND dynamics consists of a modification of the acceleration with respect to the one provided by Newtonian mechanics. In this paper we investigate whether it can be derived from a velocity-dependent deformation of the coordinates of the systems. The conclusion is that it cannot be derived this way because of the intrinsic non-local character in time of the MOND procedure. This is a feature pointed out some time ago already by Milgrom himself.
Improved the abstract, the conclusions and inserted some further new references
Nuclear and High Energy Physics, Classical Mechanic, Physics, QC1-999, FOS: Physical sciences, Equations of motion in general relativity and gravitational theory, General Relativity and Quantum Cosmology (gr-qc), Relativistic gravitational theories other than Einstein's, including asymmetric field theories, Galaxie, General Relativity and Quantum Cosmology, Classical Mechanics; Galaxies; Stars., Stars.
Nuclear and High Energy Physics, Classical Mechanic, Physics, QC1-999, FOS: Physical sciences, Equations of motion in general relativity and gravitational theory, General Relativity and Quantum Cosmology (gr-qc), Relativistic gravitational theories other than Einstein's, including asymmetric field theories, Galaxie, General Relativity and Quantum Cosmology, Classical Mechanics; Galaxies; Stars., Stars.
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