Abstract
Many alternative theories of gravity screen a Yukawa-type potential. This article shows Keplerian-type parametrization for the solution of Yukawa type potential accurate equations of motion for two nonspinning compact objects moving in an eccentric orbit, using the mean anomaly. From the analytical solution some of the post-Keplerian parameters are derived. Consequently, a bound from the Solar System is presented.
Original language | English |
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Article number | 043001 |
Journal | Physical Review D |
Volume | 106 |
Issue number | 4 |
DOIs | |
State | Published - 15 Aug 2022 |
Externally published | Yes |
ASJC Scopus subject areas
- Nuclear and High Energy Physics