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A Hamiltonian fluid-kinetic model for a two-species non-neutral plasma
Emanuele Tassi, Massimiliano Romé, Cristel Chandre

A Hamiltonian fluid-kinetic model for a two-species non-neutral plasma

Science & Mathematics Published 2014 Verification Pending

Overview & Synopsis

A model for describing the dynamics of a pure electron plasma in the presence of a population of massive charged particles is presented. The model couples the fluid dynamics of the pure electron plasma with the dynamics of the massive particle population, the latter being treated kinetically. The model is shown to possess a noncanonical Hamiltonian structure and to preserve invariants analogous to those of the two-dimensional (2D) Euler equation for an incompressible inviscid fluid, and of the Vlasov equation. The Hamiltonian structure of the model is used to derive a set of stability conditions for rotating coherent structures of the two-species system, in the case of negatively charged massive particles. According to these conditions, stability is attained if both the equilibrium distribution function of the kinetic species and the equilibrium density of the electron fluid are monotonically decreasing functions of the corresponding single-particle energies in the rotating frame. For radially confined equilibria near the axis, the stability condition corresponds to the existence of a finite interval of rotation frequencies for the reference frame, with the upper bound determined by the presence of the kinetic population.

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Document Information

Document Title A Hamiltonian fluid-kinetic model for a two-species non-neutral plasma
Author / Organization Emanuele Tassi, Massimiliano Romé, Cristel Chandre
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2014
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-89980
Original Source Link Visit Source Page on hal.science »