Large Scale Structure Formation of Normal Branch in DGP Brane World Model

Details Large Scale Structure Formation of Normal Branch in DGP Brane World Model Large Scale Structure Formation of Normal Branch in DGP Brane World Model

2007-11-15

arxiv.org/abs/0711.2513v2

Phys.Rev.D77:124031,2008

Astronomy and Astrophysics

Astrophysics

6 pages, 2 figures

Scientific paper

10.1103/PhysRevD.77.124031

In this paper, we study the large scale structure formation of the normal branch in DGP model (Dvail, Gabadadze and Porrati brane world model) by applying the scaling method developed by Sawicki, Song and Hu for solving the coupled perturbed equations of motion of on-brane and off-brane. There is detectable departure of perturbed gravitational potential from LCDM even at the minimal deviation of the effective equation of state w_eff below -1. The modified perturbed gravitational potential weakens the integrated Sachs-Wolfe effect which is strengthened in the self-accelerating branch DGP model. Additionally, we discuss the validity of the scaling solution in the de Sitter limit at late times.

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