Relativistic hydrodynamic fluctuations from an effective action: causality, stability, and the information current
Nicki Mullins, Mauricio Hippert, Lorenzo Gavassino, Jorge Noronha

TL;DR
This paper develops a covariant effective action framework for relativistic hydrodynamic fluctuations, ensuring causality and stability, and introduces a new symmetry to connect different formalisms and improve understanding of fluctuation dynamics.
Contribution
It formulates a covariant effective action for relativistic hydrodynamics incorporating causality, stability, and a novel symmetry, linking Schwinger-Keldysh and Martin-Siggia-Rose approaches.
Findings
Correlation functions exhibit physical properties within the valid regime.
A new $ ext{Z}_2$ symmetry analogous to KMS symmetry is identified.
The effective action framework clarifies the connection between different fluctuation formalisms.
Abstract
Causality is necessary for retarded Green's functions to remain retarded in all inertial frames in relativity, which ensures that dissipation of fluctuations is a Lorentz invariant concept. For first-order BDNK theories with stochastic fluctuations, introduced via the Schwinger-Keldysh formalism, we show that imposing causality and stability leads to correlation functions of hydrodynamic fluctuations that only display the expected physical properties at small frequencies and wavenumber, i.e., within the expected regime of validity of the first-order approach. For second-order theories of Israel and Stewart type, constructed using the information current such that entropy production is always non-negative, a stochastic formulation is presented using the Martin-Siggia-Rose approach where imposing causality and stability leads to correlators with the desired properties. We also show how…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Statistical Mechanics and Entropy
