Dark matter and dark energy interactions: theoretical challenges, cosmological implications and observational signatures

被引：484

作者：

Wang, B. ^{[1
]}

Abdalla, E. ^{[2
]}

Atrio-Barandela, F. ^{[3
]}

Pavon, D. ^{[4
]}

机构：

[1] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200030, Peoples R China

[2] Univ Sao Paulo, Inst Fis, BR-05508 Sao Paulo, Brazil

[3] Univ Salamanca, Fis Teor, E-37008 Salamanca, Spain

[4] Univ Autonoma Barcelona, Dept Fis, E-08193 Barcelona, Spain

来源：

REPORTS ON PROGRESS IN PHYSICS | 2016年 / 79卷 / 09期

基金：

中国国家自然科学基金; 巴西圣保罗研究基金会;

关键词：

dark matter; dark energy; interaction; BARYON ACOUSTIC-OSCILLATIONS; HUBBLE-SPACE-TELESCOPE; LARGE-SCALE STRUCTURE; DIGITAL SKY SURVEY; MICROWAVE BACKGROUND ANISOTROPIES; EQUATION-OF-STATE; PROBE WMAP OBSERVATIONS; WIGGLEZ OVERLAP REGION; GALAXY REDSHIFT SURVEY; LIGHT CURVES;

D O I：

10.1088/0034-4885/79/9/096901

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Models where dark matter and dark energy interact with each other have been proposed to solve the coincidence problem. We review the motivations underlying the need to introduce such interaction, its influence on the background dynamics and how it modifies the evolution of linear perturbations. We test models using the most recent observational data and we find that the interaction is compatible with the current astronomical and cosmological data. Finally, we describe the forthcoming data sets from current and future facilities that are being constructed or designed that will allow a clearer understanding of the physics of the dark sector.

引用

页数：49

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