Resonant sheath heating in weakly magnetized capacitively coupled plasmas due to electron-cyclotron motion

Quan-Zhi Zhang, Jing-Yu Sun, Wen-Qi Lu, Julian Schulze, Yu-Qing Guo, and You-Nian Wang
Phys. Rev. E 104, 045209 – Published 22 October 2021

Abstract

An electron heating mechanism based on a resonance between the cyclotron motion of electrons and the radio frequency sheath oscillations is reported in weakly magnetized capacitively coupled plasmas at low pressure. If half of the electron cyclotron period coincides with the radio frequency period, then electrons will coherently collide with the expanding sheath and gain substantial energy, which enhances the plasma density. A relation between the magnetic field and the driving frequency is found to characterize this resonance effect and the kinetics of electrons are revealed at resonance conditions for various driving frequencies.

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  • Received 28 October 2020
  • Revised 11 February 2021
  • Accepted 14 September 2021

DOI:https://doi.org/10.1103/PhysRevE.104.045209

©2021 American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Authors & Affiliations

Quan-Zhi Zhang1,*,†, Jing-Yu Sun1,*, Wen-Qi Lu1,‡, Julian Schulze1,2, Yu-Qing Guo1, and You-Nian Wang1

  • 1Key Laboratory of Materials Modification by Laser, Ion, and Electron Beams (Ministry of Education), School of Physics, Dalian University of Technology, Dalian 116024, China
  • 2Department of Electrical Engineering and Information Science, Ruhr-University, 44780 Bochum, Germany

  • *These authors contributed equally to this work.
  • qzzhang@dlut.edu.cn
  • luwenqi@dlut.edu.cn

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Issue

Vol. 104, Iss. 4 — October 2021

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