Electromagnetic quasinormal modes of rotating black strings and the AdS/CFT correspondence
Jaqueline Morgan, Alex S. Miranda, Vilson T. Zanchin

TL;DR
This paper studies the electromagnetic quasinormal modes of rotating black strings in AdS space and explores their dual CFT plasma behavior, revealing effects like Doppler shifts and thermalization time dilation.
Contribution
It provides a detailed analysis of electromagnetic perturbations of rotating black strings and their holographic duals, including both analytical and numerical results on quasinormal modes.
Findings
Rotation causes Doppler shifts in QNM frequencies.
Rotation affects thermalization times in the dual CFT.
Hydrodynamic regime of QNM dispersion relations is analytically characterized.
Abstract
We investigate the quasinormal spectrum of electromagnetic perturbations of rotating black strings. Among the solutions of Einstein equations in the presence of a negative cosmological constant there are asymptotically anti-de Sitter (AdS) black holes whose horizons have the topology of a cylinder. The stationary version of these AdS black holes represents rotating black strings. The conformal field theory (CFT) dual of a black string lives in a Minkowski space with a compact dimension. On the basis of the AdS/CFT duality, we interpret a CFT plasma moving with respect to the preferred rest frame introduced by the topology as the holographic dual to a rotating black string. We explore the consequences of this correspondence by investigating the electromagnetic perturbations of a black string for different rotation parameter values. As usual the electromagnetic quasinormal modes (QNM)…
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