Scalar-Tensor Dark Energy Models

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Submitted to the Proceedings of the Marcel Grossmann Conference MG11, July 2006, Berlin; 3 pages

Scientific paper

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.

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