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Ultrafast electron holes in plasma phase space dynamics

Electron holes (EH) are localized modes in plasma kinetic theory which appear as vortices in phase space. Earlier research on EH is based on the Schamel distribution function (df). A novel df is proposed here, generalizing the original Schamel df in a recursive manner. Nonlinear solutions obtained b...

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Autores principales: Jenab, Seyyed Mehdi Hosseini, Brodin, Gert, Juno, James, Kourakis, Ioannis
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8358053/
https://www.ncbi.nlm.nih.gov/pubmed/34381089
http://dx.doi.org/10.1038/s41598-021-95652-w
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author Jenab, Seyyed Mehdi Hosseini
Brodin, Gert
Juno, James
Kourakis, Ioannis
author_facet Jenab, Seyyed Mehdi Hosseini
Brodin, Gert
Juno, James
Kourakis, Ioannis
author_sort Jenab, Seyyed Mehdi Hosseini
collection PubMed
description Electron holes (EH) are localized modes in plasma kinetic theory which appear as vortices in phase space. Earlier research on EH is based on the Schamel distribution function (df). A novel df is proposed here, generalizing the original Schamel df in a recursive manner. Nonlinear solutions obtained by kinetic simulations are presented, with velocities twice the electron thermal speed. Using 1D-1V kinetic simulations, their propagation characteristics are traced and their stability is established by studying their long-time evolution and their behavior through mutual collisions.
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spelling pubmed-83580532021-08-13 Ultrafast electron holes in plasma phase space dynamics Jenab, Seyyed Mehdi Hosseini Brodin, Gert Juno, James Kourakis, Ioannis Sci Rep Article Electron holes (EH) are localized modes in plasma kinetic theory which appear as vortices in phase space. Earlier research on EH is based on the Schamel distribution function (df). A novel df is proposed here, generalizing the original Schamel df in a recursive manner. Nonlinear solutions obtained by kinetic simulations are presented, with velocities twice the electron thermal speed. Using 1D-1V kinetic simulations, their propagation characteristics are traced and their stability is established by studying their long-time evolution and their behavior through mutual collisions. Nature Publishing Group UK 2021-08-11 /pmc/articles/PMC8358053/ /pubmed/34381089 http://dx.doi.org/10.1038/s41598-021-95652-w Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Article
Jenab, Seyyed Mehdi Hosseini
Brodin, Gert
Juno, James
Kourakis, Ioannis
Ultrafast electron holes in plasma phase space dynamics
title Ultrafast electron holes in plasma phase space dynamics
title_full Ultrafast electron holes in plasma phase space dynamics
title_fullStr Ultrafast electron holes in plasma phase space dynamics
title_full_unstemmed Ultrafast electron holes in plasma phase space dynamics
title_short Ultrafast electron holes in plasma phase space dynamics
title_sort ultrafast electron holes in plasma phase space dynamics
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8358053/
https://www.ncbi.nlm.nih.gov/pubmed/34381089
http://dx.doi.org/10.1038/s41598-021-95652-w
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