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Newton's trajectories versus Mond's trajectories

GOZZI, ENNIO
2017
  • journal article

Periodico
PHYSICS LETTERS. SECTION B
Abstract
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.
DOI
10.1016/j.physletb.2017.01.002
WOS
WOS:000396438300016
Archivio
http://hdl.handle.net/11368/2890577
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85009094258
http://www.sciencedirect.com/science/article/pii/S0370269317300059
Diritti
open access
license:creative commons
license uri:http://creativecommons.org/licenses/by/3.0/it/
FVG url
https://arts.units.it/bitstream/11368/2890577/1/mond-reprint-phys.lett-b.pdf
Soggetti
  • Classical Mechanic

  • Galaxie

  • Stars.

Web of Science© citazioni
2
Data di acquisizione
Mar 25, 2024
Visualizzazioni
7
Data di acquisizione
Apr 19, 2024
Vedi dettagli
google-scholar
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