PIRSA:08060177

Video URL

https://pirsa.org/08060177

Dark Energy, Induced Gravity and Broken Scale Invariance.

(2008). Dark Energy, Induced Gravity and Broken Scale Invariance.. Perimeter Institute for Theoretical Physics. https://pirsa.org/08060177

Dark Energy, Induced Gravity and Broken Scale Invariance.. Perimeter Institute for Theoretical Physics, Jun. 06, 2008, https://pirsa.org/08060177 

          @misc{ scivideos_PIRSA:08060177,
            doi = {10.48660/08060177},
            url = {https://pirsa.org/08060177},
            author = {},
            keywords = {Quantum Fields and Strings, Particle Physics, Cosmology},
            language = {en},
            title = {Dark Energy, Induced Gravity and Broken Scale Invariance.},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2008},
            month = {jun},
            note = {PIRSA:08060177 see, \url{https://scivideos.org/pirsa/08060177}}
          }
Talk numberPIRSA:08060177
DOI10.48660/08060177
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

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 $gamma sigma^{2}R$.