Large scale structure of f(R) gravity

By Yong Song, Wayne Hu, I. Sawicki. 2006

438 citations recorded by the source corpus.

We study the evolution of linear cosmological perturbations in f(R) models of accelerated expansion in the physical frame where the gravitational dynamics are fourth order and the matter is minimally coupled. These models predict a rich and testable set of linear phenomena. For each expansion history, fixed empirically by cosmological distance measures, there exists two branches of f(R) solutions that are parametrized by B{proportional_to}d{sup 2}f/dR{sup 2}. For B 0 branch, f(R) models can reduce the large-angle CMB anisotropy, alter the shape of the linear matter power spectrum, and qualitatively change the correlations between the CMB and galaxy surveys. All of these phenomena are accessible with current and future data and provide stringent tests of general relativity on cosmological scales.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/48b6d9a3ba5f0473b470ca07e26bfca7efa4cc89

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

  1. S. Tsujikawa
  2. Lavinia Heisenberg
  3. E. Komatsu
  4. Andrey V. Kravtsov
  5. Simon D. M. White
  6. Volker Springel
  7. Salvatore Capozziello
  8. Antonio de Felice

In Nuclear and High Energy Physics

  1. S. Tsujikawa
  2. Lavinia Heisenberg
  3. Antonio de Felice
  4. Sergei D. Odintsov
  5. E. Komatsu
  6. Salvatore Capozziello
  7. Valerio Faraoni
  8. Louis Pèrenon

Citations in the corpus