Holographic superconductors in quintessence AdS black hole spacetime
Creators
- 1. Institute of Physics and Department of Physics, Hunan Normal University, Changsha, Hunan 410081 (China)
Description
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 wq of quintessence. We investigate holographic superconductors in this background and probe effects of the state parameter wq on the critical temperature Tc, the condensation formation and conductivity. The larger absolute value of wq leads to the lower critical temperature Tc 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)wq + λ± > 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. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/0264-9381/30/14/145001Additional details
Identifiers
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 30
- Journal Issue
- 14
- Journal Page Range
- [15 p.]
- ISSN
- 0264-9381
- CODEN
- CQGRDG
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44076400
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANTI DE SITTER SPACE; BLACK HOLES; CRITICAL TEMPERATURE; EINSTEIN FIELD EQUATIONS; LIMITING VALUES; MATHEMATICAL SOLUTIONS; NONLUMINOUS MATTER; SCALARS; SPACE-TIME; STRONG-COUPLING MODEL; SUPERCONDUCTORS
- Descriptors DEC
- EQUATIONS; FIELD EQUATIONS; MATHEMATICAL MODELS; MATHEMATICAL SPACE; MATTER; PARTICLE MODELS; PHYSICAL PROPERTIES; SPACE; THERMODYNAMIC PROPERTIES; TRANSITION TEMPERATURE