Test of the inverse square law through precession of orbits

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.

Authors
Kolosnitsyn N.I. 1 , Melnikov V.N. 1
Journal
General Relativity and Gravitation
Number of issue
7
Language
English
Pages
1619-1624
Status
Published
Link
External link
DOI
10.1023/B:GERG.0000032154.73097.5b
Volume
36
Year
2004
Organizations
  • 1 Ctr. Gravitation/Fundamental Metrol., VNIIMS/Inst. of Gravitation/Cosmol., Peoples' Friendship Univ. of Russia, 3-1, M. Ulyanovoi Str., 119313, Moscow, Russian Federation
Keywords
Gravitation; Newton's law; Precession of orbits
Date of creation
19.10.2018
Date of change
19.10.2018
Short link
https://repository.rudn.ru/en/records/article/record/3625/
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