f(R) theories of gravity

被引:3466
作者
Sotiriou, Thomas P. [1 ]
Faraoni, Valerio [2 ]
机构
[1] Univ Maryland, Ctr Fundamental Phys, College Pk, MD 20742 USA
[2] Bishops Univ, Dept Phys, Sherbrooke, PQ J1M 1Z7, Canada
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词
HIGHER-ORDER GRAVITY; F R GRAVITY; SPHERICALLY SYMMETRIC-SOLUTIONS; PALATINI VARIATIONAL PRINCIPLE; EINSTEIN-BOLTZMANN EQUATIONS; EXACT COSMOLOGICAL SOLUTIONS; BIG-BANG NUCLEOSYNTHESIS; HIGH-REDSHIFT SUPERNOVAE; POTENTIAL-DENSITY PAIRS; PHANTOM DARK ENERGY;
D O I
10.1103/RevModPhys.82.451
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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.
引用
收藏
页码:451 / 497
页数:47
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