Abstract

We construct a holographic dual of the Schwinger-Keldysh effective action for the dissipative low-energy dynamics of relativistic charged matter at strong coupling in a fixed thermal background. To do so, we use a mixed signature bulk spacetime whereby an eternal asymptotically anti-de Sitter black hole is glued to its Euclidean counterpart along an initial time slice in a way to match the desired double-time contour of the dual field theory. Our results are consistent with existing literature and can be regarded as a fully-ab initio derivation of a Schwinger-Keldysh effective action. In addition, we provide a simple infrared effective action for the near horizon region that drives all the dissipation and can be viewed as an alternative to the membrane paradigm approximation.

Highlights

  • One of the most active lines of research on non-equilibrium phenomena of the past two decades concerns relativistic hydrodynamics

  • The symmetries of the microscopic Schwinger-Keldysh path integral, such as unitarity and CPT invariance, have been used to constrain the form of the low-energy SchwingerKeldysh effective action and to re-derive the conventional phenomenological formulation of hydrodynamics in some limiting regimes. It was shown in ref. [31], see refs. [32, 33], how the local second law of thermodynamics can be obtained as the Noether current of a symmetry of the effective action

  • We identified the holographic dual of the degrees of freedom relevant for the fluid dynamic behavior with Wilson lines extending between the conformal boundary and the cutoff hypersurface, much in the spirit of ref. [43], see refs. [44, 45]

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Summary

The Schwinger-Keldysh effective action

Let us briefly review the main ingredients that enter the construction of Schwinger-Keldysh effective actions. In this work we are interested in the low-energy effective action Seff for charged matter at finite temperature in a fixed d-dimensional background In this case, the external sources are taken to be a pair of U(1) flavor fields AR μ and AL μ which live on two different spacetimes, dubbed as R and L, and transform as connections under two independent gauge transformations parameterized by ΛR and ΛL, AR μ → AR μ + ∂μΛR , AL μ → AL μ + ∂μΛL ,. Having defined the low-energy degrees of freedom, the most general Schwinger-Keldysh effective action Seff can be constructed requiring compatibility with the symmetries. See, e.g., refs. [20, 31]

Towards the holographic Schwinger-Keldysh effective action
The mixed signature bulk spacetime
The degrees of freedom
The effective action for diffusion from holography
The bulk piecewise solution
The holographic Schwinger-Keldysh effective action
The Schwinger-Keldysh effective action up to second order
The near-horizon region and the Schwinger-Keldysh effective action
The infrared Schwinger-Keldysh effective action
Interpretation of the infrared theory
Discussion
A Quadratic effective action for diffusion
T σ1tt0
B Details of the holographic results

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