Holographic dark energy

被引：364

作者：

Wang, Shuang ^{[1
]}

Wang, Yi ^{[2
]}

Li, Miao ^{[1
]}

机构：

[1] Sun Yat Sen Univ, Sch Phys & Astron, Guangzhou 510275, Guangdong, Peoples R China

[2] Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2017年 / 696卷

基金：

中国国家自然科学基金;

关键词：

Holographic principle; Dark energy; Cosmological observations; DIGITAL SKY SURVEY; HUBBLE-SPACE-TELESCOPE; IMPROVED COSMOLOGICAL CONSTRAINTS; FLUX-AVERAGING ANALYSIS; PROBE WMAP OBSERVATIONS; ALCOCK-PACZYNSKI TEST; COSMIC AGE PROBLEM; EQUATION-OF-STATE; OBSERVATIONAL CONSTRAINTS; POWER SPECTRUM;

D O I：

10.1016/j.physrep.2017.06.003

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We review the paradigm of holographic dark energy (HDE), which arises from a theoretical attempt of applying the holographic principle (HP) to the dark energy (DE) problem. Making use of the HP and the dimensional analysis, we derive the general formula of the energy density of HDE. Then, we describe the properties of HDE model, in which the future event horizon is chosen as the characteristic length scale. We also introduce the theoretical explorations and the observational constraints for this model. Next, in the framework of HDE, we discuss various topics, such as spatial curvature, neutrino, instability of perturbation, time-varying gravitational constant, inflation, black hole and big rip singularity. In addition, from both the theoretical and the observational aspects, we introduce the interacting holographic dark energy scenario, where the interaction between dark matter and HDE is taken into account. Furthermore, we discuss the HDE scenario in various modified gravity (MG) theories, such as Brans Dicke theory, braneworld theory, scalar tensor theory, Horava Lifshitz theory, and so on. Besides, we introduce the attempts of reconstructing various scalar-field DE and MG models from HDE. Moreover, we introduce other DE models inspired by the HP, in which different characteristic length scales are chosen. Finally, we make comparisons among various HP-inspired DE models, by using cosmological observations and diagnostic tools. (C) 2017 Elsevier B.V. All rights reserved.

引用

页码：1 / 57

页数：57

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