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Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints

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arxiv 2207.08235 v1 pith:C53JW4V2 submitted 2022-07-17 gr-qc astro-ph.EPhep-th

David Benisty This is my paper · ORCID
classification gr-qcastro-ph.EPhep-th
keywords potentialgravitysolutionyukawaaccuratealternativeanalyticalarticle
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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.

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Cited by 1 Pith paper

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  1. Big-Bang Nucleosynthesis and WIMP Dark Matter Freeze-Out as Probes of Yukawa Cosmology

    astro-ph.CO 2026-08 reject novelty 5.0 of 10

    Using BBN and WIMP relic density, the authors constrain the Yukawa gravity coupling α to about -0.017 to 0.018, with the lithium discrepancy still unexplained.

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