Scalar-Tensor Dark Energy Models Auteur(s): Gannouji Radouane, Polarski D., Ranquet Andre, Starobinsky A.A.
Conference: 11th Marcel Grossmann Meeting on General Relativity (MG 11) (Berlin, DE, 2007) Ref HAL: in2p3-00126198_v1 Ref Arxiv: astro-ph/0701650 Ref. & Cit.: NASA ADS Exporter : BibTex | endNote Résumé: 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. Commentaires: Submitted to the Proceedings of the Marcel Grossmann Conference MG11, July 2006, Berlin; 3 pages - To be published in World Scientific |