Inflationary Phase in Brans-dicke Cosmology With a Cosmological Constant
19893 pages
Published in:
- Phys.Lett.A 142 (1989) 335-337
View in:
Citations per year
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
References(5)
Figures(0)
- [1]
- [2]
- [3]
- [4]
- [5]