Evolution of cosmological perturbations in a brane-universe

Details Evolution of cosmological perturbations in a brane-universe Evolution of cosmological perturbations in a brane-universe

2000-10-10

arxiv.org/abs/hep-th/0010063v1

Phys.Rev.Lett. 86 (2001) 2212-2215

Physics

High Energy Physics

High Energy Physics - Theory

8 pages, Latex (Revtex); no figure

Scientific paper

10.1103/PhysRevLett.86.2212

The present article analyses the impact on cosmology, in particular on the evolution of cosmological perturbations, of the existence of extra-dimensions. The model considered here is that of a five-dimensional Anti-de Sitter spacetime where ordinary matter is confined to a brane-universe. The homogeneous cosmology is recalled. The equations governing the evolution of cosmological perturbations are presented in the most transparent way: they are rewritten in a form very close to the equations of standard cosmology with two types of corrections: a. corrections due to the unconventional evolution of the homogeneous solution, which change the background-dependent coefficients of the equations; b. corrections due to the curvature along the fifth dimension, which act as source terms in the evolution equations.

Affiliated with

Also associated with

No associations

Rating

Evolution of cosmological perturbations in a brane-universe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evolution of cosmological perturbations in a brane-universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of cosmological perturbations in a brane-universe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-406966