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  <title><![CDATA[Feynman rules for wave turbulence]]></title>
  <body><![CDATA[<h3>School of Physics, Nonlinear Seminar - Dr. Vladimir Rosenhaus - CUNY Graduate Center, NY</h3>

<p>It has long been known that weakly nonlinear field theories can have a late-time stationary state that is not the thermal state, but a wave turbulent state (the Kolmogorov-Zakharov state) with a far-from-equilibrium cascade of energy. We go beyond the existence of the wave turbulent state, studying fluctuations about the wave turbulent state. Specifically, we take a classical field theory with an arbitrary quartic interaction and add dissipation and Gaussian-random forcing. Employing the path integral relation&nbsp; between stochastic classical field theories and quantum field theories, we give a prescription, in terms of&nbsp; Feynman diagrams, for computing correlation functions in this system.&nbsp; We explicitly compute the two-point and four-point functions of the field to next-to-leading order in the coupling. Through an appropriate choice of forcing and dissipation, these correspond to correlation functions in the wave turbulent state. As a check, we&nbsp; reproduce the next-to-leading order term in the kinetic equation. &nbsp;The correlation functions and corrections to the KZ state that we compute should, in principle, be experimentally measurable quantities.</p>

<p><a href="https://ar5iv.org/abs/2203.08168">ar5iv.org/abs/2203.08168</a></p>
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      <value><![CDATA[School of Physics, Nonlinear Science Webinar - Dr. Vladimir Rosenhaus - CUNY Graduate Center, NY]]></value>
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      <value><![CDATA[<p>predrag.cvitanovic@physics.gatech.edu</p>
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      <url><![CDATA[https://gatech.zoom.us/j/99313032175]]></url>
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