Dynamical behavior of the extended holographic dark energy with the Hubble horizon

被引：17

作者：

Liu, Jie ^{[1
]}

Gong, Yungui ^{[1
]}

Chen, Ximing ^{[1
]}

机构：

[1] Chongqing Univ Posts & Telecommun, Coll Math & Phys, Chongqing 400065, Peoples R China

来源：

PHYSICAL REVIEW D | 2010年 / 81卷 / 08期

基金：

中国国家自然科学基金;

关键词：

EQUATION-OF-STATE; COSMOLOGICAL CONSTANT; GENERAL-RELATIVITY; 1/R GRAVITY; CONSTRAINTS; ACCELERATION; MODEL; UNIVERSE; TRANSITION; INFLATION;

D O I：

10.1103/PhysRevD.81.083536

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The extended holographic dark energy model with the Hubble horizon as the infrared cutoff avoids the problem of the circular reasoning of the holographic dark energy model. Unfortunately, it is hit with the no-go theorem. In this paper, we consider the extended holographic dark energy model with a potential, V(phi), for the Brans-Dicke scalar field. With the addition of a potential for the Brans-Dicke scalar field, the extended holographic dark energy model using the Hubble horizon as the infrared cutoff is a viable dark energy model, and the model has the dark energy dominated attractor solution.

引用

页数：7

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