Evolution of the fine-structure constant in runaway dilaton models

TL;DR

This paper investigates how the fine-structure constant evolves in string-inspired runaway dilaton models, using recent measurements to constrain the models and discussing potential observational signatures like redshift drift.

Contribution

It provides a detailed analysis of $\alpha$ evolution in runaway dilaton models and explores observational strategies to distinguish these from other varying $\alpha$ scenarios.

Findings

Current observations constrain model parameters.

Redshift drift signals can significantly differ from $\\Lambda$CDM at high redshifts.

Future measurements will tightly constrain these models.

Abstract

We study the detailed evolution of the fine-structure constant $\alpha$ in the string-inspired runaway dilaton class of models of Damour, Piazza and Veneziano. We provide constraints on this scenario using the most recent $\alpha$ measurements and discuss ways to distinguish it from alternative models for varying $\alpha$. For model parameters which saturate bounds from current observations, the redshift drift signal can differ considerably from that of the canonical $\Lambda$CDM paradigm at high redshifts. Measurements of this signal by the forthcoming European Extremely Large Telescope (E-ELT), together with more sensitive $\alpha$ measurements, will thus dramatically constrain these scenarios.