Valerio Marra and Francesca Rosati JCAP05(2005)011 doi:10.1088/1475-7516/2005/05/011
Valerio Marra and Francesca Rosati
Show affiliationsA general model for the cosmological evolution of the fine structure constant α driven by a typical quintessence scenario is presented. We consider a coupling between the quintessence scalar
and the electromagnetic kinetic term FμνFμν, given by a general function BF(
). We study the dependence of the cosmological Δα(t) upon the functional form of BF(
) and discuss the constraints imposed by the data. We find that different cosmological histories for Δα(t) are possible within the available constraints. We also find that quasar absorption spectra evidence for a time variation of α, if confirmed, is not incompatible with Oklo and meteorite limits.
E-print Number: astro-ph/0501515
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Issue 05 (May 2005)
Received 24 January 2005, accepted for publication 10 May 2005
Published 19 May 2005
Valerio Marra and Francesca Rosati JCAP05(2005)011
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