The quintessence with Abelian and non-Abelian symmetry

被引:10
|
作者
Li, XZ [1 ]
Hao, JG [1 ]
Liu, DJ [1 ]
Zhai, XH [1 ]
机构
[1] Shanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R China
来源
关键词
dark energy; quintessence; non-Abelian symmetry; metric fluctuation;
D O I
10.1142/S0217751X0301601X
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We study the perturbations on both "radial" and "angular" components of the quintessence with an internal Abelian and non-Abelian symmetry. The properties of the perturbation on the "radial" component depend on the specific potential of the model and is similiar for both Abelian and non-Abelian case. We show that the cosine-type potential is very interesting for the O(N) quintessence model and also give a critical condition of instability for the potential. While the properties of perturbations on "angular" components depend on whether the internal symmetry is Abelian or non-Abelian, which we have discussed respectively. In the non-Abelian case, the fluctuation of the "angular" component will increase rapidly with time while in the Abelian case it will not.
引用
收藏
页码:5921 / 5930
页数:10
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