Inflationary Phase in Brans-dicke Cosmology With a Cosmological Constant

1989
3 pages
Published in:
  • Phys.Lett.A 142 (1989) 335-337

Citations per year

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Abstract: (Elsevier)
It has been shown earlier that, for a perfect fluid, a perfect gas law of state, and the Robertson-Walker metric, an exponential phase in Brans-Dicke cosmology is possible, with both positive pressure and density, but not with the violated energy condition p = − ρ . We demonstrate in this paper that the inclusion of a cosmological constant into the theory does not change that picture.
  • inflation
  • cosmological constant
  • model: fluid
  • critical phenomena
  • Brans-Dicke model