4.3 Article

Coulomb collisions in strongly anisotropic plasmas II. Cyclotron cooling in laboratory pair plasmas

Journal

JOURNAL OF PLASMA PHYSICS
Volume 87, Issue 1, Pages -

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/S0022377820001233

Keywords

plasma instabilities; plasma dynamics; plasma confinement

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The study examines the distribution functions of a strongly magnetised collisional electron-positron plasma that is optically thin to cyclotron radiation on various timescales, emphasizing the anisotropy of the electron distribution function. The research also calculates the rate of radiation emission and energy loss, showing a self-accelerating process where most of the energy is lost in a few collision times. Despite deviations from Maxwellian distribution, no unstable drift waves are found in a simple case with straight field-line geometry.
The behaviour of a strongly magnetised collisional electron-positron plasma that is optically thin to cyclotron radiation is considered, and the distribution functions accessible to it on the various timescales in the system are calculated. Particular attention is paid to the limit in which the collision time exceeds the radiation emission time, making the electron distribution function strongly anisotropic. Indeed, these are the exact conditions likely to be attained in the first laboratory electron-positron plasma experiments currently being developed, which will typically have very low densities and be confined in very strong magnetic fields. The constraint of strong magnetisation adds an additional complication in that long-range Coulomb collisions, which are usually negligible, must now be considered. A rigorous collision operator for these long-range collisions has never been written down. Nevertheless, we show that the collisional scattering can be accounted for without knowing the explicit form of this collision operator. The rate of radiation emission is calculated and it is found that the loss of energy from the plasma is proportional to the parallel collision frequency multiplied by a factor that only depends logarithmically on plasma parameters. That is, this is a self-accelerating process, meaning that the bulk of the energy will be lost in a few collision times. We show that in a simple case, that of straight field-line geometry, there are no unstable drift waves in such plasmas, despite being far from Maxwellian.

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