Brane-world cosmology and inflation

MISAO SASAKI

Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan

E-mail: misao@yukawa.kyoto-u.ac.jp

Abstract. There has been substantial progress in brane-world cosmology in recent years. Much attention has been particularly paid to the second Randall{Sundrum (RS2) scenario in which a single positive-tension brane is embedded in a five-dimensional space-time, called the bulk, with a negative cosmological constant. This brane-world scenario is quite

attractive because of the non-trivial geometry in the bulk and because it successfully gives four-dimensional general relativity in the low energy limit. After reviewing basic features of the RS2 scenario, we consider a brane-world inflation model driven by the dynamics of a scalar field living in the five-dimensional bulk, the so-called bulk inflaton model. An intriguing feature of this model is that the projection of the bulk inflaton on the brane behaves just like an ordinary inflaton in four dimensions in the low energy regime, H²l² << 1, where H is the Hubble expansion rate of the brane and l² is the curvature radius of the bulk. We then discuss the cosmological perturbation on superhorizon scales in this model. We find that, even under the presence of spatial inhomogeneities, the model is indistinguishable from the standard four-dimensional inflation to O(H²l²). That is, the difference may appear only at O(H⁴l⁴).

Keywords. Brane world; cosmology; inflation.

PACS Nos 04.50.+h; 98.80.Cq