PIRSA:08060177
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Dark Energy, Induced Gravity and Broken Scale Invariance. Speaker(s): Alessandro Tronconi
Abstract: We study the cosmological evolution of an induced gravity model with a self-interacting scalar field $sigma$ 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 $gamma$ coupling to the Ricci curvature $gamma sigma^{2}R$.
Date: 06/06/2008 - 10:00 am
Collection: PASCOS 08
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