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Possible link between the changing fine-structure constant and the accelerating universe via scalar-tensor theory

Yasunori Fujii
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Abstract

In 1976, Shlyakhter showed that the Sm data from Oklo results in the upper bound on the time-variability of the fine-structure constant: $|\dotα/α| \lsim 10^{-17}{\rm y}^{-1}$, which has ever been the most stringent bound. Since the details have never been published, however, we recently re-analyzed the latest data according to Shlyakhter's recipe. We nearly re-confirmed his result. To be more precise, however, the Sm data gives either an upper-bound or an "evidence" for a changing $α$: $\dotα/α= -(0.44 \pm 0.04)\times 10^{-16}{\rm y}^{-1}$. A remark is made to a similar re-analysis due to Damour and Dyson. We also compare our result with a recent "evidence" due to Webb et al, obtained from distant QSO's. We point out a possible connection between this time-dependence and the behavior of a scalar field supposed to be responsible for the acceleration of the universe, also revealed recently.

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Yasunori Fujii. 2002-04-13. Possible link between the changing fine-structure constant and the accelerating universe via scalar-tensor theory. https://doi.org/10.1142/s0218271802002621

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