The Parameterised Post-Newtonian Limit of Bimetric Theories of Gravity
Timothy Clifton, M\'aximo Ba\~nados, Constantinos Skordis

TL;DR
This paper analyzes the post-Newtonian limit of general bimetric gravity theories, showing they can closely mimic general relativity in solar system tests and exploring the behavior of massive modes and parameter discontinuities.
Contribution
It extends the parameterized post-Newtonian framework to bimetric theories, identifying new potentials and analyzing the effects of massive modes on gravitational predictions.
Findings
Bimetric theories can evade solar system tests with sufficiently large masses.
No van Dam-Veltman-Zakharov discontinuity in gamma parameter in the massless limit.
Discontinuities in other post-Newtonian parameters occur as massive modes become massless.
Abstract
We consider the post-Newtonian limit of a general class of bimetric theories of gravity, in which both metrics are dynamical. The established parameterised post-Newtonian approach is followed as closely as possible, although new potentials are found that do not exist within the standard frame-work. It is found that these theories can evade solar system tests of post-Newtonian gravity remarkably well. We show that perturbations about Minkowski space in these theories contain both massless and massive degrees of freedom, and that in general there are two different types of massive mode, each with a different mass parameter. If both of these masses are sufficiently large then the predictions of the most general class of theories we consider are indistinguishable from those of general relativity, up to post-Newtonian order in a weak field, low velocity expansion. In the limit that the…
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