Valerio Marra and Francesca Rosati
Dipartimento di Fisica 'Galileo Galilei' and INFN, Università di Padova, via Marzolo 8, I-35126 Padova, Italy
Journal of Cosmology and Astroparticle Physics Create an alert RSS this journal
Valerio Marra and Francesca Rosati JCAP05(2005)011
A 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
Cited: by |
Refers: to
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
Wang Jian-Bo et al 2004 Chinese Phys. Lett. 21 945
S Márka et al 2002 Class. Quantum Grav. 19 1537
H Date et al 1993 J. Phys. D: Appl. Phys. 26 1211
Gérard Petit and Peter Wolf 2005 Metrologia 42 S138
Eric W. Greisen et al 2009 The Astronomical Journal 137 4718
V V Nesvizhevsky and K V Protasov 2004 Class. Quantum Grav. 21 4557
P W Martin 2002 Metrologia 39 1