Axion Homeopathy: Screening Dilaton Interactions

TL;DR

This paper introduces Axion Homeopathy, a mechanism where light axions modify dilaton interactions, allowing models to evade solar system gravity tests by converting dilaton profiles into weaker axion profiles.

Contribution

The paper proposes a novel evasion mechanism for dilaton-matter coupling bounds using axion interactions, supported by analytical solutions in SL(2,R) invariant models.

Findings

Dilaton-matter couplings can be suppressed via axion interactions.

The mechanism allows evasion of experimental bounds on scalar fields.

Analytical solutions show reduced PPN parameter deviations.

Abstract

Cosmologically active Brans-Dicke (or dilaton) scalar fields are generically ruled out by solar system tests of gravity unless their couplings to ordinary matter are much suppressed relative to gravitational strength, and this is a major hindrance when building realistic models of light dilatons coupled to matter. We propose a new mechanism for evading such bounds if matter also couples to a light axion, that exploits nonlinear target-space curvature interactions to qualitatively change how the fields respond to a gravitating source. We find that dilaton-matter couplings that would be excluded in the absence of an axion can become acceptable given an additional small axion-matter coupling, and this is possible because the axion-dilaton interactions end up converting the would-be dilaton profile into an axion profile. The trajectories of matter test bodies are then controlled by the much weaker axion-matter couplings and can easily be small enough to escape detection. We call this mechanism Axion Homeopathy because the evasion of the dilaton-coupling bounds persists for extremely small axion couplings provided only that they are nonzero. We explore the mechanism using axio-dilaton equations that are SL(2,R) invariant (as often appear in string compactifications), since for these the general solutions exterior to a spherically symmetric source can be found analytically. We use this solution to compute the relevant PPN parameters, $\beta$ and $\gamma$, and verify that their difference from unity can be much smaller than would have been true in the absence of axion-matter couplings and so can therefore evade the experimental bounds.