Evolution of density perturbations in double exponential quintessence models
arXiv:0707.2097 · doi:10.1007/s10509-007-9389-8
Abstract
In this work we investigate the evolution of matter density perturbations for quintessence models with a self-interaction potential that is a combination of exponentials. One of the models is based on the Einstein theory of gravity, while the other is based on the Brans-Dicke scalar tensor theory. We constrain the parameter space of the models using the determinations for the growth rate of perturbations derived from data of the 2-degree Field Galaxy Redshift Survey.
5 pages, 3 eps figures
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