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Kinetic Wave Turbulence

We consider a general model of Hamiltonian wave systems with triple resonances, in the standard kinetic limit of a continuum of weakly interacting dispersive waves with random phases. In this asymptotic limit we show that the correct dynamical equation for multimode amplitude distributions is not the well-known equation of Peierls but is instead a reduced equation with only a subset of the terms in that equation. The equations that we derive are the direct analogue of the Boltzmann hierarchy obtained from the BBGKY hierarchy in the low-density limit for gases. We show that the asymptotic multimode equations possess factorized solutions for factorized initial data, which correspond to preservation in time of the property of "random phases & amplitudes". The factors satisfy the equations for the 1-mode probability density functions previously derived by Jakobsen & Newell and Choi et al. We show that the factorization of the hierarchy equations implies that these quantities are self-averaging: they satisfy the wave-kinetic closure equations of the spectrum and 1-mode PDF for almost any selection of phases and amplitudes from the initial ensemble. We show that both of these clo

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Co-authorshipAuthorshipAuthorshipTopic signalTopic signalTopic signalWKinetic Wave Turbulencepreprint / 2012AGregory L. EyinkResearcherAYi-Kang ShiResearcherTmath-ph7974 worksTmath.MP7972 worksTphysics.flu-dyn4653 works
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Kinetic Wave Turbulence

preprint / 2012

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