Affiliation:
1. International School for Advanced Studies
2. National Institute of Nuclear Physics (at SISSA)
3. King's College London
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.
Subject
General Physics and Astronomy
Cited by
88 articles.
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