Nonlocal Modification of Newtonian Gravity
Hans-Joachim Blome, Carmen Chicone, Friedrich W. Hehl, Bahram, Mashhoon

TL;DR
This paper explores a nonlocal extension of Newtonian gravity within a teleparallel framework, proposing a nonlinear modification of Poisson's equation that mimics dark matter effects and analyzing its potential solar system implications.
Contribution
It introduces a novel nonlocal and nonlinear generalization of Newtonian gravity based on a scalar kernel in teleparallel gravity, linking nonlocality to dark matter simulation.
Findings
Nonlocal gravity can replicate dark matter effects.
A nonlinear Poisson equation is derived for nonlocal gravity.
Implications for solar system gravity are briefly discussed.
Abstract
The Newtonian regime of a recent nonlocal extension of general relativity (GR) is investigated. Nonlocality is introduced via a scalar "constitutive" kernel in a special case of the translational gauge theory of gravitation, namely, the teleparallel equivalent of GR. In this theory, the nonlocal aspect of gravity simulates dark matter. A nonlocal and nonlinear generalization of Poisson's equation of Newtonian gravitation is presented. The implications of nonlocality for the gravitational physics in the solar system are briefly studied.
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