Time-variability of the fine-structure constant expected from the Oklo constraint and the QSO absorption lines
arXiv:astro-ph/0307263 · doi:10.1016/j.physletb.2003.08.036
Abstract
The data from the QSO absorption lines indicating a nonzero time-variability of the fine-structure constant has been re-analyzed on the basis of a "damped-oscillator" fit, as motivated by the same type of behavior of a scalar field, dilaton, which mimics a cosmological constant to understand the accelerating universe. We find nearly as good fit to the latest data as the simple weighted mean. In this way, we offer a way to fit the more stringent result from the Oklo phenomenon, as well.
10 pages, 4 figures. Expanded section 2 and added discussion on the Re decay in section 4
References in corpus (3)
Cited by in corpus (15)
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