Hydrodynamic fluctuations, long-time tails, and supersymmetry

By P. Kovtun, Laurence G. Yaffe. 2003

146 citations recorded by the source corpus.

Hydrodynamic fluctuations at non-zero temperature can cause slow relaxation toward equilibrium even in observables which are not locally conserved. A classic example is the stress-stress correlator in a normal fluid, which, at zero wavenumber, behaves at large times as t^{-3/2}. A novel feature of the effective theory of hydrodynamic fluctuations in supersymmetric theories is the presence of Grassmann-valued classical fields describing macroscopic supercharge density fluctuations. We show that hydrodynamic fluctuations in supersymmetric theories generate essentially the same long-time power-law tails in real-time correlation functions that are known in simple fluids. In particular, a t^{-3/2} long-time tail must exist in the stress-stress correlator of N=4 supersymmetric Yang-Mills theory at non-zero temperature, regardless of the value of the coupling. Consequently, this feature of finite-temperature dynamics can provide an interesting test of the AdS/CFT correspondence. However, the coefficient of this long-time tail is suppressed by a factor of 1/N_c^2. On the gravitational side, this implies that these long-time tails are not present in the classical supergravity limit: they must instead be produced by one-loop gravitational fluctuations.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/76472bf446ea31a1480bdc4712ce88a293bee9a1

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In Astronomy and Astrophysics

  1. S. Hartnoll
  2. A. Starinets
  3. Alex Buchel
  4. S. Sachdev
  5. P. Kovtun
  6. D. Son
  7. R. Myers
  8. M. Rangamani

In Nuclear and High Energy Physics

  1. S. Hartnoll
  2. A. Starinets
  3. Christopher P. Herzog
  4. S. Sachdev
  5. Alex Buchel
  6. P. Kovtun
  7. R. Myers
  8. M. Rangamani

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