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arXiv · gr-qc/0302048

Test of inverse square law through precession of orbits

N. I. Kolosnitsyn·V. N. Melnikov
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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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N. I. Kolosnitsyn, V. N. Melnikov. 2003-02-12. Test of inverse square law through precession of orbits. https://doi.org/10.1023/b%3Agerg.0000032154.73097.5b

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