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Scalar-Tensor Dark Energy Models | R. Gannouji
; D. Polarski
; A. Ranquet
; A. A. Starobinsky
; | Date: |
23 Jan 2007 | 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. | Source: | arXiv, astro-ph/0701650 | Services: | Forum | Review | PDF | Favorites |
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