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arXiv · chao-dyn/9905014

Quasilinear theory of collisionless Fermi acceleration in a multicusp magnetic confinement geometry

Abstract

Particle motion in a cylindrical multiple-cusp magnetic field configuration is shown to be highly (though not completely) chaotic, as expected by analogy with the Sinai billiard. This provides a collisionless, linear mechanism for phase randomization during monochromatic wave heating. A general quasilinear theory of collisionless energy diffusion is developed for particles with a Hamiltonian of the form $H_0+H_1$, motion in the \emph{unperturbed} Hamiltonian $H_0$ being assumed chaotic, while the perturbation $H_1$ can be coherent (i.e. not stochastic). For the multicusp geometry, two heating mechanisms are identified --- cyclotron resonance heating of particles temporarily mirror-trapped in the cusps, and nonresonant heating of nonadiabatically reflected particles (the majority). An analytically solvable model leads to an expression for a transit-time correction factor, exponentially decreasing with increasing frequency. The theory is illustrated using the geometry of a typical laboratory experiment.

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BibTeXRIS

Robert L. Dewar, Carmen I. Ciubotariu. 1999-09-30. Quasilinear theory of collisionless Fermi acceleration in a multicusp magnetic confinement geometry. https://doi.org/10.1103/physreve.60.7400

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