Abstract
We investigate the linear growth rate of cosmological matter density perturbations in a viable model both numerically and analytically. We find that the growth rate in the scalar-tensor regime can be characterized by a simple analytic formula. We also investigate a prospect of constraining the Compton wavelength scale of the model with a future weak lensing survey.
- Received 18 November 2009
DOI:https://doi.org/10.1103/PhysRevD.81.043528
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