Electrostatic and whistler instabilities excited by an electron beam
Xin An, Jacob Bortnik, Bart Van Compernolle, Viktor Decyk, Richard, Thorne

TL;DR
This study uses a Darwin particle-in-cell simulation to analyze how electron beams excite electrostatic and whistler instabilities in space plasmas, revealing their growth, saturation, and interactions.
Contribution
It provides new insights into the excitation and competition of electrostatic and whistler instabilities by electron beams in plasma environments.
Findings
Electrostatic waves saturate quickly and can accelerate electrons.
Whistler waves are excited via Landau and cyclotron resonances.
Electrostatic instability can suppress whistler instability depending on plasma parameters.
Abstract
The electron beam-plasma system is ubiquitous in the space plasma environment. Here, using a Darwin particle-in-cell method, the excitation of electrostatic and whistler instabilities by a gyrating electron beam is studied in support of recent laboratory experiments. It is assumed that the total plasma frequency is larger than the electron cyclotron frequency . The fast-growing electrostatic beam-mode waves saturate in a few plasma oscillations by slowing down and relaxing the electron beam parallel to the background magnetic field. Upon their saturation, the finite amplitude electrostatic beam-mode waves can resonate with the tail of the background thermal electrons and accelerate them to the beam parallel velocity. The slower-growing whistler waves are excited in primarily two resonance modes: (a) through Landau resonance due to the inverted slope of the beam…
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