arXiv:0905.0730 [astro-ph.CO]AbstractReferencesReviewsResources
Analytic solution for matter density perturbations in a class of viable cosmological f(R) models
Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama
Published 2009-05-06, updated 2010-02-23Version 3
For a class of viable cosmological models in $f(R)$ gravity which deviation from the Einstein gravity decreases as a inverse power law of the Ricci scalar $R$ for large $R$, an analytic solution for density perturbations in the matter component during the matter dominated stage is obtained in terms of hypergeometric functions. An analytical expression for the matter transfer function at scales much less than the present Hubble scale is also obtained.
Comments: 11 pages; More discussion and references added, results unchanged, matches the version to be published in IJMPD; A typo in eq. (25) is fixed
Journal: Int.J.Mod.Phys.D18:1731-1740,2009
Keywords: matter density perturbations, analytic solution, viable cosmological, matter transfer function, inverse power law
Tags: journal article
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