Modified Jordan-Brans-Dicke theory with scalar current and the Eddington-Robertson gamma-parameter
John W. Moffat, Viktor T. Toth

TL;DR
This paper modifies the Jordan-Brans-Dicke theory by introducing a scalar current, resulting in a model where the Eddington-Robertson gamma-parameter equals 1, aligning with experimental constraints and preserving the weak equivalence principle.
Contribution
It proposes a scalar current modification to Jordan-Brans-Dicke theory that yields gamma=1, reconciling the theory with solar system tests and maintaining the weak equivalence principle.
Findings
Gamma parameter can be set to 1 with scalar current
Modified theory aligns with solar system measurements
Weak equivalence principle remains satisfied
Abstract
The Jordan-Brans-Dicke theory of gravitation, which promotes the gravitational constant to a dynamical scalar field, predicts a value for the Eddington-Robertson post-Newtonian parameter gamma that is significantly different from the general relativistic value of unity. This contradicts precision solar system measurements that tightly constrain gamma around 1. We consider a modification of the theory, in which the scalar field is sourced explicitly by matter. We find that this leads to a modified expression for the gamma-parameter. In particular, a specific choice of the scalar current yields gamma=1, just as in general relativity, while the weak equivalence principle is also satisfied. This result has important implications for theories that mimic Jordan-Brans-Dicke theory in the post-Newtonian limit in the solar system, including our scalar-tensor-vector modified gravity theory (MOG).
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