Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8194505 | Physics Letters B | 2009 | 4 Pages |
Abstract
We study the linear growth of matter perturbations in the DGP model with the growth index γ as a function of redshift. At the linear approximation: γ(z)âγ0+γ0â²z, we find that, for 0.2⩽Ωm,0⩽0.35, γ0 takes the value from 0.658 to 0.671, and γ0â² ranges from 0.035 to 0.042. With three low redshift observational data of the growth factor, we obtain the observational constraints on γ0 and γ0â² for the ÎCDM and DGP models and find that the observations favor the ÎCDM model but at the 1Ï confidence level both the ÎCDM and DGP models are consistent with the observations.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Xiangyun Fu, Puxun Wu, Hongwei Yu,