# Electromagnetic quasinormal modes of rotating black strings and the AdS/CFT correspondence

@article{Morgan2013ElectromagneticQM, title={Electromagnetic quasinormal modes of rotating black strings and the AdS/CFT correspondence}, author={Jaqueline Morgan and A. Santamaria Miranda and Vilson T. Zanchin}, journal={Journal of High Energy Physics}, year={2013}, volume={2013}, pages={1-24} }

A bstractWe 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…

## 14 Citations

### From quasinormal modes of rotating black strings to hydrodynamics of a moving CFT plasma

- PhysicsPhysical Review D
- 2018

A certain identification of points in a planar Schwarzschild-anti de Sitter (AdS) black hole generates a four-dimensional static black string. In turn, a rotating black string can be obtained from a…

### Separable wave equations for gravitoelectromagnetic perturbations of rotating charged black strings

- Physics
- 2015

Rotating charged black strings are exact solutions of four-dimensional Einstein–Maxwell equations with a negative cosmological constant and a non-trivial spacetime topology. According to the AdS/CFT…

### Quasinormal modes of dilaton-de Sitter black holes: scalar perturbations

- PhysicsGeneral Relativity and Gravitation
- 2016

Dilaton black hole solutions in low energy string theory (well known as GMGHS black holes) have analogue black holes with a cosmological constant derived by Gao and Zhang. Here, we study quasi normal…

### Quasinormal modes of dilaton-de Sitter black holes: scalar perturbations

- Physics
- 2016

Dilaton black hole solutions in low energy string theory (well known as GMGHS black holes) have analogue black holes with a cosmological constant derived by Gao and Zhang. Here, we study quasi normal…

### Calculating quasinormal modes of Schwarzschild anti–de Sitter black holes using the continued fraction method

- PhysicsPhysical Review D
- 2023

We investigate the scalar, gravitational, and electromagnetic quasinormal mode spectra of Schwarzschild anti-de Sitter black holes using the numerical continued fraction method. The spectra have…

### Quasi-normal modes and the area spectrum of a near extremal de Sitter black hole with conformally coupled scalar field

- Physics
- 2015

In this paper, we have studied a black hole in de Sitter space which has a conformally coupled scalar field in the background. This black hole is also known as the MTZ black hole. We have obtained…

### Black holes in massive gravity: quasi-normal modes of scalar perturbations

- Physics
- 2014

We have studied quasinormal modes of scalar perturbations of a black hole in massive gravity. The parameters of the theory, such as the mass of the black hole, the scalar charge of the black hole and…

### The correspondence between shadow and test field in a four-dimensional charged Einstein–Gauss–Bonnet black hole

- PhysicsThe European Physical Journal C
- 2021

In this paper, we investigate the photon sphere, shadow radius and quasinormal modes of a four-dimensional charged Einstein–Gauss–Bonnet black hole. The perturbation of a massless scalar field in the…

### Hydrodynamics of simply spinning black holes & hydrodynamics for spinning quantum fluids

- PhysicsJournal of High Energy Physics
- 2020

We find hydrodynamic behavior in large simply spinning five-dimensional Anti-de Sitter black holes. These are dual to spinning quantum fluids through the AdS/CFT correspondence constructed from…

### The correspondence between shadows and test fields in four-dimensional charged Einstein-Gauss-Bonnet black holes

- Physics
- 2021

In this paper, we investigate the photon sphere, shadow radius and quasinormal modes of a four-dimensional charged Einstein-Gauss-Bonnet black hole. The perturbation of a massless scalar field in the…

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