Model-independent constraints on possible modifications of Newtonian gravity

Details Model-independent constraints on possible modifications of Newtonian gravity Model-independent constraints on possible modifications of Newtonian gravity

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..61.1159t&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 61, Sept. 5, 1988, p. 1159-1162. DOE-supported research.

Astronomy and Astrophysics

Astronomy

117

Gravitational Constant, Kepler Laws, Newton Theory, Solar Gravitation, Solar System, Perihelions, Precession

Scientific paper

New model-independent constraints on possible modifications of Newtonian gravity over solar-system distance scales are presented, and their implications discussed. The constraints arise from the analysis of various planetary astrometric data sets. The results of the model-independent analysis are then applied to set limits on a variation in the l/r-squared behavior of gravity, on possible Yukawa-type interactions with ranges of the order of planetary distance scales, and on a deviation from Newtonian gravity of the type discussed by Milgrom (1983).

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