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• W2090974412 abstract "We study the cosmological evolution of an induced gravity model with a self-interacting scalar field σ and in the presence of matter and radiation. Such model leads to Einstein gravity plus a cosmological constant as a stable attractor among homogeneous cosmologies and is therefore a viable dark-energy (DE) model for a wide range of scalar field initial conditions and values for its positive γ coupling to the Ricci curvature γσ2R." @default.
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• W2090974412 date "2008-01-01" @default.
• W2090974412 modified "2023-10-02" @default.
• W2090974412 title "Dark energy, induced gravity and broken scale invariance" @default.
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• W2090974412 doi "https://doi.org/10.1016/j.physletb.2007.11.053" @default.
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