Modified Newtonian dynamics habitats within the solar system

@inproceedings{Bekenstein2006ModifiedND,
  title={Modified Newtonian dynamics habitats within the solar system},
  author={Jacob Bekenstein and Jo{\~a}o Magueijo},
  year={2006}
}
MOdified Newtonian Dynamics (MOND) is an interesting alternative to the presence of dark matter in galaxies. We here examine the possibility that mild or even strong MOND behavior may become evident well inside the solar system, in particular, near saddle points of the total gravitational potential. Whereas in Newtonian theory tidal stresses are finite at saddle points, they are expected to diverge in MOND, and to remain distinctly large inside a sizable oblate ellipsoid around the saddle point… CONTINUE READING