Signature of the interaction between dark energy and dark matter in galaxy clusters

被引:130
作者
Abdalla, Elcio [1 ]
Abramo, L. Raul [1 ]
Sodre, Laerte, Jr. [2 ]
Wang, Bin [3 ]
机构
[1] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
[2] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Dept Astron, BR-05508090 Sao Paulo, Brazil
[3] Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China
基金
巴西圣保罗研究基金会;
关键词
OBSERVATIONAL CONSTRAINTS; COSMOLOGICAL CONSTANT; SUPERNOVAE; UNIVERSE; MASS;
D O I
10.1016/j.physletb.2009.02.008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the influence of ail interaction between dark energy and dark matter upon the dynamics of galaxy clusters. We obtain file general Layser-Irvine equation in the presence of interactions, and find how, in that case. the virial theorem stands corrected. Using optical, X-ray and weak lensing data from 33 relaxed galaxy clusters, we put constraints on the strength of the coupling between the dark sectors. Available data Suggests that this coupling is small but positive, indicating that dark energy might be decaying into dark matter. Systematic effects between the several mass estimates, however, should be better known, before definitive conclusions oil the magnitude and significance of this coupling could be established. (C) 2009 Published by Elsevier B.V.
引用
收藏
页码:107 / 110
页数:4
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