Particle-in-cell simulations of the relaxation of electron beams in inhomogeneous solar wind plasmas
J.O. Thurgood, D. Tsiklauri

TL;DR
This study uses fully kinetic particle-in-cell simulations to investigate how background density irregularities in the solar wind affect electron beam relaxation and Langmuir wave dynamics, confirming theoretical predictions.
Contribution
First fully kinetic PIC simulations of electron beam relaxation in inhomogeneous plasmas, validating quasi-linear and Hamiltonian models with new insights into wave behavior.
Findings
In homogeneous plasma, Langmuir waves are generated at resonance and lead to wave packet growth.
In inhomogeneous plasma, high-energy electrons are produced, unlike in homogeneous cases.
Density fluctuations cause refraction of Langmuir waves, generating backward waves.
Abstract
Previous theoretical considerations of electron beam relaxation in inhomogeneous plasmas have indicated that the effects of the irregular solar wind may account for the poor agreement of homogeneous modelling with the observations. Quasi-linear theory and Hamiltonian models based on Zakharov's equations have indicated that when a level of density fluctuations is above a given threshold, density irregularities act to de-resonate the beam-plasma interaction, restricting Langmuir wave growth on the expense of beam energy. This work presents the first fully kinetic particle-in-cell (PIC) simulations of beam relaxation under the influence of density irregularities. We aim to independently determine the influence of background inhomogeneity on the beam-plasma system, and to test theoretical predictions and alternative models using a fully kinetic treatment. We carry out 1D PIC simulations of…
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