Interacting two-fluid viscous dark energy models in a non-flat universe

被引：0
|
作者：
Hassan Amirhashchi [1 ]
Anirudh Pradhan [2 ]
Hishamuddin Zainuddin [3 ]
机构：
[1] Young Researchers Club,Mahshahr Branch,Islamic Azad University
[2] Department of Mathematics,Hindu Post-graduate College
[3] Laboratory of Computational Sciences and Mathematical Physics,Institute for Mathematical Research,University Putra Malaysia
来源：
Research in Astronomy and Astrophysics | 2013年 / 13卷 / 02期
关键词：
cosmology:theory — dark energy — viscous fluid;
D O I：
暂无
中图分类号：
P145.9 [其他];
学科分类号：
070401 ;
摘要：
We study the evolution of the dark energy parameter within the scope of a spatially non-flat and isotropic Friedmann-Robertson-Walker model filled with barotropic fluid and bulk viscous stresses.We have obtained cosmological solutions that do not have a Big Rip singularity,and concluded that in both non-interacting and interacting cases the non-flat open Universe crosses the phantom region.We find that during the evolution of the Universe,the equation of state for dark energy ωD changes from ωDeff>-1 to ωDeff<-1,which is consistent with recent observations.
引用
收藏
页码：129 / 138
页数：10
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