Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution

被引:1936
|
作者
Nojiri, S. [1 ,2 ,3 ]
Odintsov, S. D. [4 ,5 ,7 ,8 ]
Oikonomou, V. K. [6 ,7 ]
机构
[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
[2] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan
[3] High Energy Accelerator Res Org KEK, KEK Theory Ctr, Oho 1-1, Tsukuba, Ibaraki 3050801, Japan
[4] CSIC, IEEC, Inst Ciencies Espai, Carrer Can Magrans S-N, Barcelona 08193, Spain
[5] Passeig Co, ICREA, Barcelona 08010, Spain
[6] Tomsk State Univ Control Syst & Radioelect TUSUR, Lab Theoret Cosmol, Tomsk 634050, Russia
[7] Tomsk State Pedag Univ, Tomsk 634061, Russia
[8] Compl Univ Monte S Angelo, INFN Sez Napoli, Edificio G,Via Cinthia, I-80126 Naples, Italy
关键词
EQUATION-OF-STATE; OSCILLATING DARK ENERGY; GAUSS-BONNET THEORY; F R THEORIES; COSMOLOGICAL CONSTANT; F(R) GRAVITY; GENERAL-RELATIVITY; NEUTRON-STAR; BIG RIP; PHANTOM COSMOLOGY;
D O I
10.1016/j.physrep.2017.06.001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We systematically review some standard issues and also the latest developments of modified gravity in cosmology, emphasizing on inflation, bouncing cosmology and late time acceleration era. Particularly, we present the formalism of standard modified gravity theory representatives, like F(R), F(G) and F(T) gravity theories, but also several alternative theoretical proposals which appeared in the literature during the last decade. We emphasize on the formalism developed for these theories and we explain how these theories can be considered as viable descriptions for our Universe. Using these theories, we present how a viable inflationary era can be produced in the context of these theories, with the viability being justified if compatibility with the latest observational data is achieved. Also we demonstrate how bouncing cosmologies can actually be described by these theories. Moreover, we systematically discuss several qualitative features of the dark energy era by using the modified gravity formalism, and also we critically discuss how a unified description of inflation with dark energy era can be described by solely using the modified gravity framework. Finally, we also discuss some astrophysical solutions in the context of modified gravity, and several qualitative features of these solutions. The aim of this review is to gather the different modified gravity techniques and form a virtual modified gravity "toolbox", which will contain all the necessary information on inflation, dark energy and bouncing cosmologies in the context of the various forms of modified gravity. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 104
页数:104
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