Impact of Lorentz Violation Models on Exoplanets’ Dynamics

Many exoplanets have been detected by the radial velocity method, according to which motion of a binary system around its center mass can produce periodical variation Doppler effect light emitted host star. These variations are influenced both Newtonian and non-Newtonian perturbations dominant inverse-square acceleration; accordingly, exoplanetary systems lend themselves testing theories gravity alternative general relativity. In this paper, we consider impact Standard Model Extension (a model that be used test all possible Lorentz violations) on perturbation suggest suitable exoplanets’ configurations improvements in detection techniques may contribute obtaining new constraints parameters.