Further understanding the interaction between dark energy and dark matter: current status and future directions

被引：18

作者：

Wang, B. ^{[1
]}

Abdalla, E. ^{[2
]}

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

Pavon, D. ^{[4
]}

机构：

[1] Shanghai Jiao Tong Univ, Sch Aeronaut & Astronaut, Shanghai 200240, Peoples R China

[2] Univ Sao Paulo, Inst Fis, Sao Paulo, SP, Brazil

[3] Univ Salamanca, Fis Teor, Plaza Merced, Salamanca, Spain

[4] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain

来源：

REPORTS ON PROGRESS IN PHYSICS | 2024年 / 87卷 / 03期

关键词：

dark energy; dark matter; interaction; theoretical models; observations; BARYON ACOUSTIC-OSCILLATIONS; COSMOLOGICAL PARAMETER CONSTRAINTS; VIABLE F(R) GRAVITY; N-BODY SIMULATIONS; INITIAL CONDITIONS; HUBBLE CONSTANT; POWER SPECTRUM; OBSERVATIONAL CONSTRAINTS; MASSIVE NEUTRINOS; BLACK-HOLES;

D O I：

10.1088/1361-6633/ad2527

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The interaction between dark matter and dark energy (DE) can be incorporated into field theory models of DE that have proved successful in alleviating the coincidence problem. We review recent advances in this field, including new models and constraints from different astronomical data sets. We show that interactions are allowed by observations and can reduce the current tensions among different measurements of cosmological parameters. We extend our discussion to include constraints from non-linear effects and results from cosmological simulations. Finally, we discuss forthcoming multi-messenger data from current and future observational facilities that will help to improve our understanding of the interactions within the dark sector.

引用

页数：24

共 370 条

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