Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in the non-flat universe

被引：40

作者：

Karami, K. ^{[1
,2
]}

Khaledian, M. S. ^{[1
]}

Jamil, Mubasher ^{[3
]}

机构：

[1] Univ Kurdistan, Dept Phys, Pasdaran St, Sanandaj, Iran

[2] RIAAM, Maragha, Iran

[3] NUST, CAMP, Islamabad, Pakistan

来源：

PHYSICA SCRIPTA | 2011年 / 83卷 / 02期

关键词：

PROBE WMAP OBSERVATIONS; COSMOLOGICAL CONSTANT; K-ESSENCE; CONSTRAINTS; TACHYON; SUPERNOVAE; MAPS;

D O I：

10.1088/0031-8949/83/02/025901

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Here we consider the entropy-corrected version of the holographic dark energy (DE) model in the non-flat universe. We obtain the equation of state parameter in the presence of interaction between DE and dark matter. 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 entropy-corrected holographic DE model.

引用

页数：7

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