• DOI:10.1103/PhysRevD.98.026006
• Corpus ID: 119465669

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

@article{Mamani2018FromQM,
  title={From quasinormal modes of rotating black strings to hydrodynamics of a moving CFT plasma},
  author={Luis A. H. Mamani and Jaqueline Morgan and A. Santamaria Miranda and Vilson T. Zanchin},
  journal={Physical Review D},
  year={2018}
}

• Luis A. H. Mamani, Jaqueline Morgan, +1 author V. Zanchin
• Published 4 April 2018
• Physics
• Physical Review D

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 static one by means of an `illegitimate coordinate transformation', a local boost in the compact direction. On the basis of the gauge/gravity duality, these black strings are dual to rotating thermal states of a strongly interacting conformal field theory (CFT) that lives on a cylinder. In this work, we obtain the complete quasinormal mode (QNM) spectrum of the gravitational perturbations of rotating black strings. Analytic solutions for the dispersion relations are found in the hydrodynamic limit, characterized by fluctuations with wavenumber and frequency much smaller than the Hawking temperature of the string (or the temperature in the CFT dual description). We obtain these dispersion relations both by studying the gravitational perturbations of rotating black strings and by investigating the hydrodynamic fluctuations of a moving fluid living on the boundary of the AdS spacetime. Relativistic effects like the Doppler shift of the frequencies, wavelength contraction, and dilation of the thermalization time are shown explicitly in such a regime. We also investigate the behavior of a sound wave propagating in a viscous fluid for several values of the rotation parameter. The numerical solutions for the fundamental QNMs show a crossover (a transition) from a hydrodynamic-like behavior to a linear relativistic scaling for large wavenumbers. Additionally, we find a new family of QNMs which are purely damped in the zero wavenumber limit and that does not follow as a continuation of QNMs of the static black string, but that appears to be closely related to the algebraically special perturbation modes.