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.

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

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Cited by in corpus (2)

• Nonlinear Electromagnetic Quasinormal Modes and Hawking Radiation of A Regular Black Hole with Magnetic Charge
• Vortex structure deformation of rotating Lifshitz Holographic Superconductors