Effective Action for Relativistic Hydrodynamics: Fluctuations, Dissipation, and Entropy Inflow

TL;DR

This paper develops a comprehensive effective field theory framework for relativistic hydrodynamics, incorporating fluctuations, dissipation, and entropy flow, ensuring consistency with thermodynamic principles and symmetries.

Contribution

It introduces a novel superspace formalism and symmetry principles to derive hydrodynamic equations and fluctuations from a unified effective action.

Findings

Reproduces hydrodynamic constitutive relations consistent with the second law

Predicts non-Gaussian hydrodynamic fluctuations

Provides a covariant superspace formalism for hydrodynamics

Abstract

We present a detailed and self-contained analysis of the universal Schwinger-Keldysh effective field theory which describes macroscopic thermal fluctuations of a relativistic field theory, elaborating on our earlier construction in arXiv:1511.07809. We write an effective action for appropriate hydrodynamic Goldstone modes and fluctuation fields, and discuss the symmetries to be imposed. The constraints imposed by fluctuation-dissipation theorem are manifest in our formalism. Consequently, the action reproduces hydrodynamic constitutive relations consistent with the local second law at all orders in the derivative expansion, and captures the essential elements of the eightfold classification of hydrodynamic transport of arXiv:1502.00636. We demonstrate how to recover the hydrodynamic entropy and give predictions for the non-Gaussian hydrodynamic fluctuations. The basic ingredients of our construction involve (i) doubling of degrees of freedom a la Schwinger-Keldysh, (ii) an emergent thermal gauge symmetry associated with entropy which is encapsulated in a Noether current a la Wald, and (iii) a BRST/topological supersymmetry imposing the fluctuation-dissipation theorem a la Parisi-Sourlas. The overarching mathematical framework for our construction is provided by the balanced equivariant cohomology of thermal translations, which captures the basic constraints arising from the Schwinger-Keldysh doubling, and the thermal Kubo-Martin-Schwinger relations. All these features are conveniently implemented in a covariant superspace formalism. An added benefit is that the second law can be understood as being due to entropy inflow from the Grassmann-odd directions of superspace.