Abstract

We study fluctuations around equilibrium in a class of strongly interacting non-conformal plasmas using holographic techniques. In particular we calculate the quasi-normal mode spectrum of black hole backgrounds that approach to Chamblin-Reall plasmas in the IR. In a specific limit, related to the exact linear-dilaton background in string theory, we observe that the plasma approaches criticality and we obtain the quasi-normal spectrum analytically. We regulate the critical limit by gluing the IR geometry that corresponds to the non-conformal plasma to a part of AdS space-time in the UV. Near criticality, we find two sets of quasi-normal modes, related to the IR and UV parts of the geometry. In the critical limit, the quasi-normal modes accumulate to form a branch cut in the correlators of the energy-momentum tensor on the real axis of the complex frequency plane.

Highlights

  • Many applications of holographic duality concern systems around a critical point, where there is scale invariance

  • In a previous paper [4] we studied time-dependent solutions of this model corresponding to boost-invariant flow, and found that the system has a slower approach to equilibrium than in the conformal case

  • In the UV-completed geometry we can take the critical limit ξ → ∞ as there is no issue with the boundary conditions

Read more

Summary

INTRODUCTION

Many applications of holographic duality concern systems around a critical point, where there is scale invariance. We see that when we approach the critical point, the quasinormal modes become closely spaced and their imaginary part decreases, until eventually they form a branch cut on the real axis, even as the temperature remains finite at the critical point We argue that this behavior signals a breakdown of hydrodynamics, as there are modes that decay more slowly than the hydrodynamic fluctuations. It is not clear if there is a dual theory exactly at the critical point (it has been suggested that it could correspond to an order-disorder transition in a spin model [9]). There is another set of modes, starting at a higher frequency whose imaginary part is only mildly frequency-dependent, which we associate with the slice of the AdS space

QUASINORMAL MODES OF THE CR PLASMA
UV COMPLETION
APPROACH TO CRITICALITY
CONCLUSIONS
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.