Holographic view of cosmological perturbations

被引：8
|
作者：
Soda, J [1 ]
Kanno, S
机构：
[1] Kyoto Univ, FIHS, Dept Fundamental Sci, Kyoto 6068501, Japan
[2] Kyoto Univ, Grad Sch Human & Environm Studies, Kyoto 6068501, Japan
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2003年 / 283卷 / 04期
关键词：
D O I：
10.1023/A:1022519910504
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
引用
收藏
页码：639 / 644
页数：6
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