Holographic Dark Energy with Extended Chaplygin Gas Model

G. S. Khadekar, Aina Gupta
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引用次数: 1

Abstract

Abstract In this paper we consider a correspondence between holographic dark energy density and extended Chaplygin gas energy density proposed by Pourhassan and Kahya [2014] (Advances in High Energy Physics, 231452, 2014) in FRW universe. We solve the Friedmann equation and investigate the be- haviour of cosmological parameters and also we reconstruct the potential and dynamics of the scalar field which describe the extended Chaplygin gas cosmology.
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扩展Chaplygin气体模型的全息暗能量
本文考虑了FRW宇宙中全息暗能量密度与Pourhassan和Kahya [2014] (Advances In High energy Physics, 231452, 2014)提出的扩展Chaplygin气体能量密度的对应关系。我们求解了弗里德曼方程,研究了宇宙学参数的be-行为,并重建了描述扩展的查普金气体宇宙学的标量场的势和动力学。
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