Scalar-Tensor Dark Energy Models
Astrophysics
2016-11-15 v1
Abstract
We present here some recent results concerning scalar-tensor Dark Energy models. These models are very interesting in many respects: they allow for a consistent phantom phase, the growth of matter perturbations is modified. Using a systematic expansion of the theory at low redshifts, we relate the possibility to have phantom like DE to solar system constraints.
Cite
@article{arxiv.astro-ph/0701650,
title = {Scalar-Tensor Dark Energy Models},
author = {R. Gannouji and D. Polarski and A. Ranquet and A. A. Starobinsky},
journal= {arXiv preprint arXiv:astro-ph/0701650},
year = {2016}
}
Comments
Submitted to the Proceedings of the Marcel Grossmann Conference MG11, July 2006, Berlin; 3 pages