The quintessence with Abelian and non-Abelian symmetry
被引:10
作者:
Li, XZ
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h-index: 0
机构:
Shanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R ChinaShanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R China
Li, XZ
[1
]
Hao, JG
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机构:
Shanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R ChinaShanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R China
Hao, JG
[1
]
Liu, DJ
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h-index: 0
机构:
Shanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R ChinaShanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R China
Liu, DJ
[1
]
Zhai, XH
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h-index: 0
机构:
Shanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R ChinaShanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R China
Zhai, XH
[1
]
机构:
[1] Shanghai Normal Univ, Shanghai United Ctr Astrophys, Shanghai 200234, Peoples R China
来源:
INTERNATIONAL JOURNAL OF MODERN PHYSICS A
|
2003年
/
18卷
/
32期
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.