Holographic superconductors in quintessence AdS black hole spacetime

被引:37
|
作者
Chen, Songbai [1 ,2 ,3 ]
Pan, Qiyuan [1 ,2 ,3 ]
Jing, Jiliang [1 ,2 ,3 ]
机构
[1] Hunan Normal Univ, Inst Phys, Changsha 410081, Hunan, Peoples R China
[2] Hunan Normal Univ, Dept Phys, Changsha 410081, Hunan, Peoples R China
[3] Hunan Normal Univ, Key Lab Low Dimens Quantum Struct & Quantum Contr, Minist Educ, Changsha 410081, Hunan, Peoples R China
基金
中国国家自然科学基金;
关键词
QUASI-NORMAL MODES; COSMOLOGICAL CONSTANT; ENERGY COMPONENT; STRING THEORY; CONSEQUENCES; EQUATION; QUANTUM;
D O I
10.1088/0264-9381/30/14/145001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a solution of Einstein equations describing a d-dimensional planar quintessence anti-de Sitter (AdS) black hole which depends on the state parameter w(q) of quintessence. We investigate holographic superconductors in this background and probe effects of the state parameter w(q) on the critical temperature T-c, the condensation formation and conductivity. The larger absolute value of w(q) leads to the lower critical temperature T-c and the higher ratio between the gap frequency in conductivity to the critical temperature for the condensates. Moreover, we also find that for the scalar condensate there exists an additional constraint condition originating from the quintessence (d - 1) w(q) + lambda(+/-) > 0 for the operators O-+/-, respectively. Our results show that the scalar condensation is harder to form and the occurrence of the holographic dual superconductor needs the stronger coupling in the quintessence AdS black hole spacetime.
引用
收藏
页数:15
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