Interacting viscous entropy-corrected holographic scalar field models of dark energy with time-varying G in modified FRW cosmology

被引：0

作者：

Farzin Adabi ^{[1
]}

Kayoomars Karami ^{[2
]}

Fereshte Felegary ^{[2
]}

Zohre Azarmi ^{[2
]}

机构：

[1] Department of Physics,Sanandaj Branch,Islamic Azad University

[2] Department of Physics,University of Kurdistan

来源：

ResearchinAstronomyandAstrophysics | 2012年 / 12卷 / 01期

关键词：

cosmology:dark energy — cosmological parameters;

D O I：

暂无

中图分类号：

P159 [宇宙学];

学科分类号：

070401 ;

摘要：

We study the entropy-corrected version of the holographic dark energy(HDE) model in the framework of modified Friedmann-Robertson-Walker cosmology.We consider a non-flat universe filled with an interacting viscous entropy-corrected HDE(ECHDE) with dark matter.Also included in our model is the case of the variable gravitational constant G.We obtain the equation of state and the deceleration parameters of the interacting viscous ECHDE.Moreover,we reconstruct the potential and the dynamics of the quintessence,tachyon,K-essence and dilaton scalar field models according to the evolutionary behavior of the interacting viscous ECHDE model with time-varying G.

引用

页码：26 / 38

页数：13

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