Reconstructing an interacting holographic polytropic gas model in a non-flat FRW universe

被引：27
作者：
Karami, K. [1 ,2 ]
Abdolmaleki, A. [1 ]
机构：
[1] Univ Kurdistan, Dept Phys, Pasdaran St, Sanandaj, Iran
[2] RIAAM, Maragha, Iran
来源：
PHYSICA SCRIPTA | 2010年 / 81卷 / 05期
关键词：
AGEGRAPHIC DARK ENERGY; PROBE WMAP OBSERVATIONS; SCALAR FIELD MODELS; EQUATION-OF-STATE; COSMOLOGICAL CONSTANT; CONSTRAINTS; TACHYON; PHANTOM; MATTER; DYNAMICS;
D O I：
10.1088/0031-8949/81/05/055901
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We study the correspondence between the interacting holographic dark energy and the polytropic gas model of dark energy in a non-flat FRW universe. This correspondence allows one to reconstruct the potential and the dynamics for the scalar field of the polytropic model, which describe accelerated expansion of the universe.
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页数：6
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