Abstract (EN):
We study the evolution of the fine-structure constant, a, induced by non-linear density perturbationsin the context of the simplest class of quintessence models with a non-minimal coupling to the electromagnetic field, in which the gauge kinetic function is Taylor-expanded up to linear order. We show that the results obtained using the spherical infall model for an infinite wavelength inhomogeneity are inconsistent with the results of a local linearized gravity study and we argue in favour of the second approach. We also discuss recent claims that the value of a inside virialized regions could be significantly different from the background one on the basis of these findings.
Language:
English
Type (Professor's evaluation):
Scientific
No. of pages:
11