Electron Velocity Distributions in a Partially Ionized Gas
- 15 January 1960
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 117 (2), 343-354
- https://doi.org/10.1103/PhysRev.117.343
Abstract
The Boltzmann method is applied to the problem of calculating the electron velocity distribution in a partially ionized gas. Inelastic collisions with neutral molecules as well as random two-body Coulomb interactions are included. The latter are treated by use of the Fokker-Planck equation. Application is made to a hydrogen plasma subjected to an externally applied electric field. Static solutions are obtained, by numerical means, as a function of the ionization degree, and the classical gas discharge parameter, . It is shown that the evolution of the electron velocity distribution function from that characteristic of a poorly ionized gas to the Maxwellian distribution occurs over a very large range in ionization degree. Several applications are also made to energy relaxation phenomena, and the electrical conductivity is evaluated.
Keywords
This publication has 13 references indexed in Scilit:
- Fokker-Planck Equation for an Inverse-Square ForcePhysical Review B, 1957
- Transport Phenomena in a Completely Ionized GasPhysical Review B, 1953
- A Collective Description of Electron Interactions: II. CollectiveIndividual Particle Aspects of the InteractionsPhysical Review B, 1952
- On Brownian motion, Boltzmann’s equation, and the Fokker-Planck equationQuarterly of Applied Mathematics, 1952
- The Electrical Conductivity of an Ionized GasPhysical Review B, 1950
- Electron Velocity Distribution Function in High Frequency Alternating Fields Including Electronic InteractionsPhysical Review B, 1949
- Electronic Interaction in Electrical Discharges in GasesPhysical Review B, 1949
- Energy Distribution of Electrons in High Frequency Gas DischargesPhysical Review B, 1946
- Stochastic Problems in Physics and AstronomyReviews of Modern Physics, 1943
- The Time of Relaxation of Stellar Systems.The Astrophysical Journal, 1941