paper

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

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