Characterizing the linear growth rate of cosmological density perturbations in an f(R) model

Tatsuya Narikawa and Kazuhiro Yamamoto
Phys. Rev. D 81, 043528 – Published 16 February 2010; Erratum Phys. Rev. D 81, 129903 (2010)

Abstract

We investigate the linear growth rate of cosmological matter density perturbations in a viable f(R) 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 f(R) model with a future weak lensing survey.

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  • Received 18 November 2009

DOI:https://doi.org/10.1103/PhysRevD.81.043528

©2010 American Physical Society

Erratum

Authors & Affiliations

Tatsuya Narikawa and Kazuhiro Yamamoto

  • Department of Physical Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan

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Issue

Vol. 81, Iss. 4 — 15 February 2010

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