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Testing MOND in the Solar System · Around

2011

Testing MOND in the Solar System

Blanchet, Luc, Novak, Jerome

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The Modified Newtonian Dynamics (MOND) generically predicts a violation of the strong version of the equivalence principle.

As a result the gravitational dynamics of a system depends on the external gravitational field in which the system is embedded.
This so-called external field effect is shown to imply the existence of an anomalous quadrupolar correction, along the direction of the external galactic field, in the gravitational potential felt by planets in the Solar System.
We compute this effect by a numerical integration of the MOND equation in the presence of an external field, and deduce the secular precession of the perihelion of planets induced by this effect.

Built on

Methods of celestial mechanics
D. Brouwer and G.M. Clemence · 1961
Earlier work this paper cites.
Astrophys. J
M. Milgrom · 1983
Earlier work this paper cites.
Astrophys. J
J.D. Bekenstein and M. Milgrom · 1984
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Mon. Not. Roy. Astron. Soc
K. Begeman, A. Broeils, and R. Sanders · 1991
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Ann. Rev. Astron. Astrophys
R.H. Sanders and S. McGaugh · 2002
Earlier work this paper cites.

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