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• W2140171368 abstract "We examine the variation of the fine structure constant in the context of a two-field quintessence model. We find that, for solutions that lead to a transient late period of accelerated expansion, it is possible to fit the data arising from quasar spectra and comply with the bounds on the variation of $ensuremath{alpha}$ from the Oklo reactor, meteorite analysis, atomic clock measurements, cosmic microwave background radiation, and big bang nucleosynthesis. That is more difficult if we consider solutions corresponding to a late period of permanent accelerated expansion." @default.
• W2140171368 created "2016-06-24" @default.
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• W2140171368 date "2004-11-16" @default.
• W2140171368 modified "2023-09-27" @default.
• W2140171368 title "Time evolution of the fine structure constant in a two-field quintessence model" @default.
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• W2140171368 doi "https://doi.org/10.1103/physrevd.70.107304" @default.
• W2140171368 hasPublicationYear "2004" @default.
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