Interaction between modified Chaplygin gas and ghost dark energy in the presence of extra dimensions

被引：11

作者：

Khurshudyan, M. ^{[1
]}

Sadeghi, J. ^{[2
]}

Hakobyan, M. ^{[3
,4
]}

Farahani, H. ^{[2
]}

Myrzakulov, R. ^{[5
]}

机构：

[1] Yerevan State Univ, Dept Theoret Phys, Yerevan 0025, Armenia

[2] Mazandaran Univ, Dept Phys, Babol Sar, Iran

[3] AI Alikhanyan Natl Sci Lab, Yerevan, Armenia

[4] Yerevan State Univ, Dept Nucl Phys, Yerevan 0025, Armenia

[5] Eurasian Natl Univ, Eurasian Int Ctr Theoret Phys, Astana 010008, Kazakhstan

来源：

EUROPEAN PHYSICAL JOURNAL PLUS | 2014年 / 129卷 / 06期

关键词：

COSMOLOGICAL CONSTANT; MODEL; VISCOSITY; DENSITY; MATTER;

D O I：

10.1140/epjp/i2014-14119-x

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

In this paper, we consider three different models of dark energy in higher-dimensional space-time and discuss some cosmological parameters numerically. The first model is a single-component universe including viscous varying modified Chaplygin gas. In the second model, we consider a two-component universe including viscous varying modified Chaplygin gas and ghost dark energy. In the third model, we consider another two-component universe including viscous modified cosmic Chaplygin gas and ghost dark energy. In the cases of two-component fluids we also consider the possibility of interaction between components.

引用

页数：8

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