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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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Showing 2007Show all

9 papers · 1 filter

gr-qc2007★ 298 cited

Solar system and equivalence principle constraints on f(R) gravity by chameleon approach

Salvatore Capozziello, Shinji Tsujikawa

We study constraints on f(R) dark energy models from solar system experiments combined with experiments on the violation of equivalence principle. When the mass of an equivalent sc…

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…

hep-th2007★ 72 cited

Prospects of inflation in delicate D-brane cosmology

Sudhakar Panda, M. Sami, Shinji Tsujikawa

We study D-brane inflation in a warped conifold background that includes brane-position dependent corrections for the nonperturbative superpotential. Instead of stabilizing the vol…

astro-ph2007★ 297 cited

Matter density perturbations and effective gravitational constant in modified gravity models of dark energy

Shinji Tsujikawa

We derive the equation of matter density perturbations on sub-horizon scales for a general Lagrangian density f(R, phi, X) that is a function of a Ricci scalar R, a scalar field ph…

astro-ph2007★ 281 cited

Phantom crossing, equation-of-state singularities, and local gravity constraints in f(R) models

Luca Amendola, Shinji Tsujikawa

We identify the class of f(R) dark energy models which have a viable cosmology, i.e. a matter dominated epoch followed by a late-time acceleration. The deviation from a LambdaCDM m…