Holographic View of Cosmological Perturbations
arXiv:gr-qc/0209086 · doi:10.1023/A:1022519910504
Abstract
The cosmological perturbation theory is revisited from the holographic point of view. In the case of the single brane model, it turns out that the AdS/CFT correspondence plays an important role. In the case of the two-brane model, it is shown that the effective equations of motion becomes the quasi-scalar-tensor gravity. It is also demonstrated that the radion anisotropy gives the CMB fluctuations through the Sachs-Wolfe effect.
6 pages, Talk presented at the JENAM 2002 Workshop on Varying Fundamental Constants, Porto, 5th September 2002. To be published in the Conference Proceedings
References in corpus (4)
Cited by in corpus (11)
- Brane-World Gravity
- Brane-world gravity
- Low Energy Effective Action for Dilatonic Braneworld --A Formalism for Inflationary Braneworld--
- Radionic Non-uniform Black Strings
- Rotating Black String and Effective Teukolsky Equation in Braneworld
- AdS/CFT on the brane
- A four-dimensional description of five-dimensional N-brane models
- Gravitational Interactions in a General Multibrane Model
- Non-linear Gravity on Branes and Effective Action
- Gravitational Waves from Rotating Black Strings
- Inflationary Braneworld Driven By Bulk Scalar Field