Anisotropy and inflation in Bianchi I brane worlds
arXiv:gr-qc/0303096 · doi:10.1088/0264-9381/21/4/005
Abstract
After a more general assumption on the influence of the bulk on the brane, we extend some conclusions by Maartens et al. and Santos et al. on the asymptotic behavior of Bianchi I brane worlds. As a consequence of the nonlocal anisotropic stresses induced by the bulk, in most of our models, the brane does not isotropize and the nonlocal energy does not vanish in the limit in which the mean radius goes to infinity. We have also found the intriguing possibility that the inflation due to the cosmological constant might be prevented by the interaction with the bulk. We show that the problem for the mean radius can be completely solved in our models, which include as particular cases those in the references above.
10 pages, improved discussion on the likeliness of non-isotropization, completed list of references, matches version to appear in Class. Quantum Grav
References in corpus (10)
- Cosmology and Brane Worlds: A Review
- Bulk effects in the cosmological dynamics of brane-world scenarios
- Kaluza-Klein anisotropy in the CMB
- The shear dynamics in Bianchi I cosmological model on the brane
- A generalisation of the Heckmann - Schucking cosmological solution
- Bianchi IX Brane-world Cosmologies
- Braneworld cosmological models with anisotropy
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Cited by in corpus (14)
- Brane-World Gravity
- Brane-world gravity
- Theory of cosmological perturbations in an anisotropic universe
- Predictions from an anisotropic inflationary era
- Dynamics of Brane-World Cosmological Models
- Brane cosmology with an anisotropic bulk
- Thick Brane Isotropization in a Generalized 5D Anisotropic Standing Wave Braneworld Model
- Large-scale perturbations on the brane and the isotropy of the cosmological singularity
- Anisotropic Inflation in a 5D Standing Wave Braneworld and Dimensional Reduction
- Braneworld Isotropization and Magnetic Fields
- Anisotropic brane cosmologies with exponential potentials
- Brane-world Cosmologies with non-local bulk effects
- The Dynamics of Brane-World Cosmological Models
- Cosmic No Hair for Braneworlds with a Bulk Dilaton Field