Test of inverse square law through precession of orbits

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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References in corpus (3)

• Sub-millimeter tests of the gravitational inverse-square law: A search for "large" extra dimensions
• Exact solutions in multidimensional gravity with antisymmetric forms
• Constraints to a Yukawa gravitational potential from laser data to LAGEOS satellites

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• Long range gravity tests and the Pioneer anomaly
• Variations of constants as a test of gravity, cosmology and unified models
• Thermodynamic Properties of Yukawa-Schwarzschild Black Hole in Non-commutative Gauge Gravity