The evolution of density perturbations in two quintessence models
Astrophysics
2007-05-23 v1
Abstract
In this work we investigate the evolution of matter density perturbations for two different quintessence models. One of them is based on the Einstein theory of gravity, while the other is based on the Brans-Dicke scalar tensor theory. We show that it is possible to 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.
Cite
@article{arxiv.astro-ph/0403031,
title = {The evolution of density perturbations in two quintessence models},
author = {Tame Gonzalez and Rolando Cardenas},
journal= {arXiv preprint arXiv:astro-ph/0403031},
year = {2007}
}
Comments
11 pages, 2 figures