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Scalar-Tensor Dark Energy Models

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.

preprint2007arXivOpen access
R. GannoujiD. PolarskiA. RanquetA. A. Starobinsky
astro-ph
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Open access4 authors1 topic
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R. GannoujiD. PolarskiA. RanquetA. A. Starobinsky

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