Dynamics of dark energy with a coupling to dark matter

被引:145
作者
Boehmer, Christian G. [1 ]
Caldera-Cabral, Gabriela [2 ]
Lazkoz, Ruth [3 ]
Maartens, Roy [2 ]
机构
[1] UCL, Dept Math, London WC1E 6BT, England
[2] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England
[3] Euskal Herriko Unibertsitatea, Fis Teorikoa, Bilbao 48080, Spain
基金
英国科学技术设施理事会;
关键词
D O I
10.1103/PhysRevD.78.023505
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Dark energy and dark matter are the dominant sources in the evolution of the late universe. They are currently only indirectly detected via their gravitational effects, and there could be a coupling between them without violating observational constraints. We investigate the background dynamics when dark energy is modeled as exponential quintessence and is coupled to dark matter via simple models of energy exchange. We introduce a new form of dark sector coupling, which leads to a more complicated dynamical phase space and has a better physical motivation than previous mathematically similar couplings.
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页数:8
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