Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints
arXiv:2207.08235 · doi:10.1103/PhysRevD.106.043001
Abstract
Many alternative theories of gravity screens a Yukawa-type potential. This article shows Keplerian-type parametrization as a solution of Yukawa type potential accurate equations of motion for two non-spinning compact objects moving in an eccentric orbit. A bound from the solar system is presented.
Accepted for Phys Rev D
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