Scalar-Tensor Dark Energy Models
arXiv:astro-ph/0701650 · doi:10.1142/9789812834300_0259
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.
Submitted to the Proceedings of the Marcel Grossmann Conference MG11, July 2006, Berlin; 3 pages