Variation of the fine structure constant caused by expansion of the Universe
Anton A. Lipovka, Ivan A. Cardenas

TL;DR
This paper estimates the universe's expansion causes a tiny but potentially measurable variation in the fine structure constant, linking it to energy losses in physical systems and discussing implications for precision experiments.
Contribution
It introduces a model connecting universe expansion to fine structure constant variation and evaluates its magnitude, proposing that current experiments could detect this change.
Findings
Estimated variation (d alpha)/alpha = 1.10^{-18} per second
Variation is within experimental detection limits in a few years
Double clock experiments are unsuitable for measuring this variation
Abstract
In present paper we evaluate the fine structure constant variation, that should take place as the Universe expands and its curvature is changed adiabatically. Such variation of the fine structure constant is attributed to an energy losses by an extended physical system (consist of baryonic component and electromagnetic field) due to expansion of our Universe. Obtained ratio (d alpha)/alpha = 1. 10{-18} (per second) is only five times smaller than actually reported experimental limit on this value. For this reason obtained variation can probably be measured within a couple of years. To argue the correctness of our approach we calculate the Planck constant as adiabatic invariant of the electromagnetic field propagated on a manifold characterized by slowly varied geometry, in the framework of the pseudo- Riemannian geometry. Finally we discuss the double clock experiment based on Al+ and…
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