Accelerating cosmologies in Lovelock gravity with dilaton
arXiv:0903.0083 · doi:10.2174/1874381101003010037
Abstract
For the description of the Universe expansion, compatible with observational data, a model of modified gravity - Lovelock gravity with dilaton - is investigated. D-dimensional space with 3- and (D-4)-dimensional maximally symmetric subspaces is considered. Space without matter and space with perfect fluid are under test. In various forms of the theory under way (third order without dilaton and second order - Einstein-Gauss-Bonnet gravity - with dilaton and without it) stationary, power-law, exponential and exponent-of-exponent form cosmological solutions are obtained. Last two forms include solutions which are clear to describe accelerating expansion of 3-dimensional subspace. Also there is a set of solutions describing cosmological expansion which does not tend to isotropization in the presence of matter.
23 pages
References in corpus (4)
- Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Thermodynamics of Rotating Charged Black Branes in Third Order Lovelock Gravity and the Counterterm Method
- Stationary vs. singular points in an accelerating FRW cosmology derived from six-dimensional Einstein-Gauss-Bonnet gravity