Clustering of dark energy -: art. no. 047302

被引:5
|
作者
Alvarenga, FG [1 ]
Fabris, JC [1 ]
Gonçalves, SVB [1 ]
Tadaiesky, G [1 ]
机构
[1] Univ Fed Espirito Santo, Dept Fis, BR-29060900 Vitoria, ES, Brazil
关键词
D O I
10.1103/PhysRevD.66.047302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A cosmological model with pressureless matter and a fluid of negative pressure is studied. At the perturbative level, fluctuations of both fluids are considered. It is shown that, at least at very large scales, the fluid of negative pressure, which represents the dark energy content of the universe, clusters like the dust fluid. Numerical integration reveals that this behavior may also occur at scales smaller than the Hubble radius.
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页数:3
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