On the structure and statistical theory of turbulence of extended magnetohydrodynamics
George Miloshevich, Manasvi Lingam, Philip J. Morrison

TL;DR
This paper explores the statistical and structural properties of turbulence in extended magnetohydrodynamics (XMHD), revealing cascade behaviors and spectral characteristics relevant to space and astrophysical plasmas using Hamiltonian methods.
Contribution
It introduces a Hamiltonian framework for XMHD turbulence, analyzes cascade directions, and extends ideal MHD results to include Hall drift and electron inertia effects.
Findings
Inverse cascade of magnetic helicity in Hall MHD range
Direct cascade of spectral quantities in inertial MHD range
Verification of Liouville's theorem for XMHD
Abstract
Recent progress regarding the noncanonical Hamiltonian formulation of extended magnetohydrodynamics (XMHD), a model with Hall drift and electron inertia, is summarized. The advantages of the Hamiltonian approach are invoked to study some general properties of XMHD turbulence, and to compare them against their ideal MHD counterparts. For instance, the helicity flux transfer rates for XMHD are computed, and Liouville's theorem for this model is also verified. The latter is used, in conjunction with the absolute equilibrium states, to arrive at the spectra for the invariants, and to determine the direction of the cascades, e.g., generalizations of the well-known ideal MHD inverse cascade of magnetic helicity. After a similar analysis is conducted for XMHD by inspecting second order structure functions and absolute equilibrium states, a couple of interesting results emerge. When cross…
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