Drift wave turbulence in a dense semiclassical magnetoplasma
Alexander Kendl, Padma K. Shukla

TL;DR
This paper develops a semiclassical model for drift wave turbulence in dense magnetized plasmas, revealing how quantum effects influence instability growth rates and turbulence characteristics at nanoscale levels.
Contribution
It introduces a novel semiclassical nonlinear collisional drift wave model that incorporates quantum statistical pressure and Bohm force effects.
Findings
Quantum effects increase drift wave instability growth rates.
Quantum effects introduce de Broglie length screening.
Nanoscale turbulence behavior is significantly affected by quantum influences.
Abstract
A semiclassical nonlinear collisional drift wave model for dense magnetized plasmas is developed and solved numerically. The effects of fluid electron density fluctuations associated with quantum statistical pressure and quantum Bohm force are included, and their influences on the collisional drift wave instability and the resulting fully developed nanoscale drift wave turbulence are discussed. It is found that the quantum effects increase the growth rate of the collisional drift wave instability, and introduce a finite de Broglie length screening on the drift wave turbulent density perturbations. The relevance to nanoscale turbulence in nonuniform dense magnetoplasmas is discussed.
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