Density operator approach to turbulent flows in plasma and atmospheric fluids
Konstantin G. Zloshchastiev

TL;DR
This paper introduces a wave-mechanical statistical framework for modeling dissipation and instabilities in 2D turbulent flows of plasmas and atmospheric fluids, revealing new energy and enstrophy exchange mechanisms.
Contribution
It develops a novel density operator approach using a non-Hermitian Hamiltonian to describe turbulence as a macroscopic wave phenomenon, extending beyond traditional wave kinetic models.
Findings
Predicts mechanisms of energy transfer between drift waves and zonal flows.
Shows the system's evolution depends on environmental effects on stability.
Provides a phase-space formulation including conservation laws.
Abstract
We formulate a statistical wave-mechanical approach to describe dissipation and instabilities in two-dimensional turbulent flows of magnetized plasmas and atmospheric fluids, such as drift and Rossby waves. This is made possible by the existence of Hilbert space, associated with the electric potential of plasma or stream function of atmospheric fluid. We therefore regard such turbulent flows as macroscopic wave-mechanical phenomena, driven by the non-Hermitian Hamiltonian operator we derive, whose anti-Hermitian component is attributed to an effect of the environment. Introducing a wave-mechanical density operator for the statistical ensembles of waves, we formulate master equations and define observables: such as the enstrophy and energy of both the waves and zonal flow as statistical averages. We establish that our open system can generally follow two types of time evolution,…
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