%0 Conference Proceedings
%T Scalar-Tensor Dark Energy Models
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%A Gannouji, R.
%A Polarski, D.
%A Ranquet, A.
%A Starobinsky, A.A.
%Z Submitted to the Proceedings of the Marcel Grossmann Conference MG11, July 2006, Berlin; 3 pages - To be published in World Scientific
%< avec comité de lecture
%Z PTA/07-32
%( Proceedings of the 11th Marcel Grossmann Meeting on General Relativity
%B 11th Marcel Grossmann Meeting on General Relativity (MG 11)
%C Berlin, Germany
%Y KLEINERT, H and JANTZEN R.T.
%I World Scientific
%V B
%P 1794-1796
%8 2006-07-23
%D 2006
%Z astro-ph/0701650
%Z Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]Conference papers
%X 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.
%G English
%L in2p3-00126198
%U https://hal.in2p3.fr/in2p3-00126198
%~ IN2P3
%~ LPTA
%~ CNRS
%~ UNIV-MONTP2
%~ UNIV-MONTPELLIER
%~ UM1-UM2