Dark matter vs . modifications of the gravitational inverse-square law . Results from planetary motion in the solar system

@inproceedings{Sereno2006DarkMV,
  title={Dark matter vs . modifications of the gravitational inverse-square law . Results from planetary motion in the solar system},
  author={Mauro Sereno and Ph. Jetzer},
  year={2006}
}
Dark matter or modifications of the Newtonian inverse-square law in the solar system are studied with accurate planetary astrometric data. From extra-perihelion precession and possible changes in the third Kepler's law, we get an upper limit on the local dark matter density, ρ DM < ∼ 3×10 −16 kg/m 3 at the 2-σ confidence level. Variations in the 1/r 2 behavior are considered in the form of either a possible Yukawa-like interaction or a modification of gravity of MOND type. Up to scales of 10 11… CONTINUE READING

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