Test of inverse square law through precession of orbits
arXiv:gr-qc/0302048 · doi:10.1023/B:GERG.0000032154.73097.5b
Abstract
Using precession of orbits due to non-Newtonian interaction between two celestial bodies and modern tracking data of satellites, planets and a pulsar we obtain new more precise limits on possible Yukawa-type deviations from the Newton law in planets (satellites)radii ranges.
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