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19992026
most citedf(R) theories

3.9k citations · 23.3k across the 206 of their papers we have counts for

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29 papers · 1 filter

astro-ph2008★ 24 cited

Second-order matter density perturbations and skewness in scalar-tensor modified gravity models

Takayuki Tatekawa, Shinji Tsujikawa

We study second-order cosmological perturbations in scalar-tensor models of dark energy that satisfy local gravity constraints, including f(R) gravity. We derive equations for matt…

astro-ph2008★ 49 cited

Generic estimates for magnetic fields generated during inflation including Dirac-Born-Infeld theories

Kazuharu Bamba, Nobuyoshi Ohta, Shinji Tsujikawa

We estimate the strength of large-scale magnetic fields produced during inflation in the framework of Dirac-Born-Infeld (DBI) theories. This analysis is sufficiently general in the…

astro-ph2008★ 68 cited

The effect of modified gravity on weak lensing

Shinji Tsujikawa, Takayuki Tatekawa

We study the effect of modified gravity on weak lensing in a class of scalar-tensor theory that includes gravity as a special case. These models are designed to satisfy loca…

astro-ph2008★ 162 cited

Constraints on scalar-tensor models of dark energy from observational and local gravity tests

Shinji Tsujikawa, Kotub Uddin, Shuntaro Mizuno +2

We construct a family of viable scalar-tensor models of dark energy (DE) which possess a phase of late-time acceleration preceded by a standard matter era, while at the same time s…

astro-ph2007★ 124 cited

Density perturbations in f(R) gravity theories in metric and Palatini formalisms

Shinji Tsujikawa, Kotub Uddin, Reza Tavakol

We make a detailed study of matter density perturbations in both metric and Palatini formalisms in theories whose Lagrangian density is a general function, f(R), of the Ricci scala…

astro-ph2007★ 445 cited

Observational signatures of f(R) dark energy models that satisfy cosmological and local gravity constraints

Shinji Tsujikawa

We discuss observational consequences of f(R) dark energy scenarios that satisfy local gravity constraints (LGC) as well as conditions of the cosmological viability. The model we s…