Abstract

Using generalized hydrodynamics (GHD), we develop the Euler hydrodynamics of classical integrable field theory. Classical field GHD is based on a known formalism for Gibbs ensembles of classical fields, that resembles the thermodynamic Bethe ansatz of quantum models, which we extend to generalized Gibbs ensembles (GGEs). In general, GHD must take into account both solitonic and radiative modes of classical fields. We observe that the quasi-particle formulation of GHD remains valid for radiative modes, even though these do not display particle-like properties in their precise dynamics. We point out that because of a UV catastrophe similar to that of black body radiation, radiative modes suffer from divergences that restrict the set of finite-average observables; this set is larger for GGEs with higher conserved charges. We concentrate on the sinh-Gordon model, which only has radiative modes, and study transport in the domain-wall initial problem as well as Euler-scale correlations in GGEs. We confirm a variety of exact GHD predictions, including those coming from hydrodynamic projection theory, by comparing with Metropolis numerical evaluations.

Highlights

  • Classical field generalized hydrodynamics (GHD) is based on a known formalism for Gibbs ensembles of classical fields, that resembles the thermodynamic Bethe ansatz of quantum models, which we extend to generalized Gibbs ensembles (GGEs)

  • We explicitly compare GHD predictions with Metropolis simulations of classically fluctuating initial states evolved deterministically with the field’s equations of motion. We study both the partitioning protocol [31,32,33,34,35,36,37]

  • The results presented above follow from i) generalizing the results of [51, 69], for the sineGordon and sinh-Gordon models, to arbitrary models in arbitrary GGEs, and ii) combining with the results of [7, 8] in order to get the hydrodynamics

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Summary

Introduction

Integrability has provided the backbone for a wide array of exact results in theoretical physics, in as diverse frameworks as quantum chains and classical fields. We explicitly compare GHD predictions with Metropolis simulations of classically fluctuating initial states evolved deterministically with the field’s equations of motion We study both the partitioning protocol (or domain wall initial condition) [31,32,33,34,35,36,37] Our study provides in particular the first numerical tests for the recent GHD constructions of Euler-scale correlation functions in integrable models [18, 25]. Appendix C contains the numerical methods needed to solve the GHD and to directly simulate the model

GHD of classical fields
Formulation
The quasi-particle description
Averages of densities and currents
Euler-scale correlations
The sinh-Gordon model
GGE of the sinh-Gordon model and UV finiteness
UV finiteness
Conclusions
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