Holographic Superconductors in a Rotating Spacetime

Abstract

We consider holographic superconductors in a rotating black string spacetime. In view of the mandatory introduction of the $A_{\phi }$ component of the vector potential we are left with three equations to be solved. Their solutions show that the effect of the rotating parameter $a$ influences the critical temperature $T_c$ and the conductivity $\sigma$ in a simple but not trivial way.

arXiv comment9 pages, 5 figures, paper completely rewritten and improved. Version to appear in EPJC

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• Scalar field propagation in braneworld black hole scenario obtained from Nash theorem
• A new rotating axionic AdS${}_4$ black hole dressed with a scalar field
• Effects of background rotation and anisotropy in the holographic description of type-II superconductors
• Novel five-dimensional rotating Lifshitz black holes with electric and axionic charges