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f(R) theories of gravity

Thomas P. Sotiriou* and Valerio Faraoni†

Thomas P. Sotiriou*

  • Center for Fundamental Physics, University of Maryland, College Park, Maryland 20742-4111, USA

Valerio Faraoni†

  • Physics Department, Bishop’s University, 2600 College Street, Sherbrooke, Québec, Canada J1M 1Z7

  • *Present address: Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK. T.Sotiriou@damtp.cam.ac.uk
  • †vfaraoni@ubishops.ca
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Rev. Mod. Phys. 82, 451 – Published 1 March, 2010

DOI: https://doi.org/10.1103/RevModPhys.82.451

Abstract

Modified gravity theories have received increased attention lately due to combined motivation coming from high-energy physics, cosmology, and astrophysics. Among numerous alternatives to Einstein’s theory of gravity, theories that include higher-order curvature invariants, and specifically the particular class of f(R) theories, have a long history. In the last five years there has been a new stimulus for their study, leading to a number of interesting results. Here f(R) theories of gravity are reviewed in an attempt to comprehensively present their most important aspects and cover the largest possible portion of the relevant literature. All known formalisms are presented—metric, Palatini, and metric affine—and the following topics are discussed: motivation; actions, field equations, and theoretical aspects; equivalence with other theories; cosmological aspects and constraints; viability criteria; and astrophysical applications.

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