Lectures on hydrodynamic fluctuations in relativistic theories
Pavel Kovtun
TL;DR
These lectures analyze hydrodynamic fluctuations in relativistic fluids by combining linear response, stochastic hydrodynamics, and an effective action viewpoint. They derive retarded correlation functions $G^R_{ab}(\omega,\mathbf{k})$ and associated Kubo formulas for transport coefficients $(\eta,\zeta,\sigma)$, uncovering non-analytic contributions (e.g. $|\omega|^{1/2}$ in $d=3$ and $\ln|\omega|$ in $d=2$) that signal breakdowns of the derivative expansion. A field-theoretic formulation with auxiliary fields and ghosts enables systematic treatment of mode interactions, including one-loop corrections and renormalization-group flows in low dimensions. The results illuminate how hydrodynamic fluctuations alter transport, constrain effective theories, and bear on strongly coupled systems such as the quark-gluon plasma and quantum critical regimes, highlighting the necessity to augment derivative expansions with fluctuation physics.
Abstract
These are pedagogical lecture notes on hydrodynamic fluctuations in normal relativistic fluids. The lectures discuss correlation functions of conserved densities in thermal equilibrium, interactions of the hydrodynamic modes, an effective action for viscous fluids, and the breakdown of the derivative expansion in hydrodynamics.
