An Interacting model of Dark Energy in Brans-Dicke theory

Feb 18, 2014
10 pages
Published in:
  • Astrophys.Space Sci. 351 (2014) 651-660
  • Published: 2014
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Abstract: (arXiv)
In this paper it is shown that in non-minimally coupled Brans-Dicke theory containing a self-interacting potential, a suitable conformal transformation can automatically give rise to an interaction between the normal matter and the Brans-Dicke scalar field. Considering the scalar field in the Einstein frame as the quintessence matter, it has been shown that such a non-minimal coupling between the matter and the scalar field can give rise to a late time accelerated expansion for the universe preceded by a decelerated expansion for very high values of the Brans-Dicke parameter ω\omega. We have also studied the observational constraints on the model parameters considering the Hubble and Supernova data.
Note:
  • 12 pages, 15 figures. Accepted for publication in Astrophysics and Space Science
  • Dark energy
  • Brans-Dicke scalar field
  • Conformal transformation
  • field theory: scalar
  • transformation: conformal
  • expansion: acceleration
  • expansion: deceleration
  • coupling: nonminimal
  • Brans-Dicke model
  • quintessence