Brane-cosmology dynamics with induced gravity
arXiv:gr-qc/0308046 · doi:10.1023/B:GERG.0000016922.72972.67
Abstract
The Friedmann equations for a brane with induced gravity are analyzed and compared with the standard general relativity and Randall-Sundrum cases. Randall-Sundrum gravity modified the early universe dynamics, whereas induced gravity changes the late universe evolution. The early and late time limits are investigated. Induced gravity effects can contribute to late-universe acceleration. This conditions for this are found. Qualitative analysis is given for a range of scalar field potentials.
14 pages, 25 eps figures, higher-resolution figures can be obtained from the author. Minor corrections. To appear in Gen.Rel.Grav. 36 (2004)
References in corpus (1)
Cited by in corpus (15)
- Brane-World Gravity
- Brane-world gravity
- Late acceleration and crossing in induced gravity
- Self accelerating solutions in a DGP brane with a scalar field trapped on it: the dynamical systems perspective
- Hysteresis in the Sky
- Bulk scalar field in DGP braneworld cosmology
- Interacting Tsallis agegraphic dark energy in DGP Braneworld Cosmology
- Phantom Mimicry on the Normal Branch of a DGP-inspired Braneworld Scenario with Curvature Effect
- Gauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the Brane
- Dynamical System Analysis of Randall-Sundrum Model with Tachyon Field on the Brane
- Non linear equation of state and effective phantom divide in brane models
- Dvali-Gabadadze-Porrati Cosmology in Bianchi I brane
- The Stability Analysis of Brane Induced Gravity with Quintessence Field on the Brane with a Gaussian Potential
- Stability Analysis of DGP Brane-world Model with Agegraphic Dark Energy
- Evolution of the density parameter in the anisotropic DGP cosmology