Hot-electron zero-field mobility and diffusion in rare-gas moderators

Darryl R. A. McMahon and Bernie Shizgal
Phys. Rev. A 31, 1894 – Published 1 March 1985
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Abstract

An efficient discrete-ordinate method of solution of the time-dependent Boltzmann equation is employed in the calculation of the zero-field electron mobility and diffusion coefficients for hot-electron thermalization in rare-gas moderators. The discrete-ordinate method is modified to permit a rescaling of the quadrature points. This procedure is somewhat analogous to the two-temperature-moment methods employed in the theoretical analysis of electron swarms. The time-dependent transport coefficients are given as a sum of exponential decay terms characterized by the discrete eigenvalues of the Lorentz-Fokker-Planck operator for elastic electron-atom collisions. For argon, krypton, and xenon, the time dependence is strongly influenced by the Ramsauer-Townsend minimum and leads to maxima in the transient mobility and diffusion coefficient. Helium and neon with hard-sphere-like cross sections exhibit transient mobilities which initially are below the thermal zero-field mobility and then increase to the thermal mobilities as the electron distribution approaches equilibrium. The transient mobility for cross sections with Ramsauer minima are sufficiently sensitive to the details of the cross sections such that it may be feasible to distinguish between different cross sections experimentally. The calculations also indicate that the transient mobility is insensitive to the initial distribution function. A nonequilibrium phenomenon not previously recognized is the possibility of a negative transient mobility which occurs provided that the momentum-transfer cross section increases sufficiently rapidly with energy.

  • Received 7 June 1984

DOI:https://doi.org/10.1103/PhysRevA.31.1894

©1985 American Physical Society

Authors & Affiliations

Darryl R. A. McMahon and Bernie Shizgal

  • Department of Chemistry, University of British Columbia, Vancouver, British Columbia V6T1Y6

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Vol. 31, Iss. 3 — March 1985

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