Dynamical study of the hyperextended scalar-tensor theory in the empty Bianchi type I model
arXiv:gr-qc/0309086 · doi:10.1088/0264-9381/17/7/307
Abstract
The dynamics of the hyperextended scalar-tensor theory in the empty Bianchi type I model is investigated. We describe a method giving the sign of the first and second derivatives of the metric functions whatever the coupling function. Hence, we can predict if a theory gives birth to expanding, contracting, bouncing or inflationary cosmology. The dynamics of a string inspired theory without antisymetric field strength is analysed. Some exact solutions are found.
18 pages, 3 figures
References in corpus (6)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Scalar-Tensor Cosmologies and their Late Time Evolution
- On the Asymptotic Behaviour of Cosmological Models in Scalar-Tensor Theories of Gravity
- Observation of Cosmic Acceleration and Determining the Fate of the Universe
- Asymptotic and Exact Solutions of Perfect-Fluid Scalar-Tensor Cosmologies