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    Quasilinear thermalization of collision-poor plasmas by noncollective fluctuations

    R. Schlickeiser1,2,* and M. Kröger3,†

    • 1Institut für Theoretische Physik, Lehrstuhl IV: Weltraum- und Astrophysik, Ruhr-Universität Bochum, D-44780 Bochum, Germany
    • 2Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 15, D-24118 Kiel, Germany
    • 3Magnetism and Interface Physics & Computational Polymer Physics, Department of Materials, ETH Zurich, Leopold-Ruzicka-Weg 4, Zurich CH-8093, Switzerland

    • *Contact author: rsch@tp4.rub.de
    • †Contact author: mk@mat.ethz.ch

    Phys. Rev. E 112, 025209 – Published 21 August, 2025

    DOI: https://doi.org/10.1103/p4xz-8ltl

    Abstract

    The observed Maxwellian velocity distribution functions in plasmas and the fact that the rate of elastic electron-electron collisions is many orders of magnitude smaller than the electron plasma frequency have been a long-standing puzzle. Here, we present a mechanism for efficient thermalization in collision-poor unmagnetized plasmas, which resolves this puzzle. The competition between the momentum losses of plasma particles by spontaneously emitting high-frequency non-collective fluctuations and the momentum diffusion of these particles in their self-generated fluctuating electric field fluctuations provides the Maxwellian particle distribution function. The mechanism is self-regulating, providing electron temperatures of about 107K, and it is applicable to fully ionized plasmas with electron densities below 1027cm−3.

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