Isotropisation of Generalized Scalar-Tensor theory plus a massive scalar field in the Bianchi type I model
arXiv:gr-qc/0309094 · doi:10.1088/0264-9381/18/15/304
Abstract
In this paper we study the isotropisation of a Generalized Scalar-Tensor theory with a massive scalar field. We find it depends on a condition on the Brans-Dicke coupling function and the potential and show that asymptotically the metric functions always tend toward a power or exponential law of the proper time. These results generalise and unify these of De Sitter in the case of a cosmological constant and of Cooley and Kitada in the case of an exponential potential.
10 pages
References in corpus (1)
Cited by in corpus (8)
- The stability of modified gravity models
- Scalar fields properties for flat galactic rotation curves
- Noether Symmetry of the Hyperextended Scalar Tensor theory for the FLRW models
- Isotropisation of Bianchi class A models with a minimally coupled scalar field and a perfect fluid
- Bianchi type IX asymptotical behaviours with a massive scalar field: chaos strikes back
- Isotropisation of flat homogeneous Bianchi type I model with a non minimally coupled and massive scalar field
- Isotropisation of flat homogeneous universes with scalar fields
- Isotropisation of Bianchi class A models with curvature for a minimally coupled scalar tensor theory