Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma
The plasma modes are significantly influenced by the simple or/and molecular anions. The reciprocity of beam and tri-ion electron (TIE) plasmas is modeled by the kinetic theory. The set of Vlasov–Poisson equation is solved and decomposed by the Laguerre–Gaussian function under paraxial approximation...
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Format: | Article |
Language: | English |
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AIP Publishing LLC
2022-10-01
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Series: | AIP Advances |
Online Access: | http://dx.doi.org/10.1063/5.0014682 |
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author | Kashif Arshad Stefaan Poedts Alaa Dahshan |
author_facet | Kashif Arshad Stefaan Poedts Alaa Dahshan |
author_sort | Kashif Arshad |
collection | DOAJ |
description | The plasma modes are significantly influenced by the simple or/and molecular anions. The reciprocity of beam and tri-ion electron (TIE) plasmas is modeled by the kinetic theory. The set of Vlasov–Poisson equation is solved and decomposed by the Laguerre–Gaussian function under paraxial approximation. The beam plasma expedites unstable twisted modes (UTMs) in the TIE plasma. The UTM or instability is calibrated via axial and azimuthal wave numbers, wind speed, and its growth essence. The qualitative and quantitative anatomy of the instability threshold is also predicted. Our model is eminently applicable to the space plasmas and has been applied to the Ar+–F−–SF6− and Xe+–F−–SF6− electron plasmas, specifically. |
first_indexed | 2024-04-12T10:56:15Z |
format | Article |
id | doaj.art-0cab8c584ca34226befd09e00b5b1c31 |
institution | Directory Open Access Journal |
issn | 2158-3226 |
language | English |
last_indexed | 2024-04-12T10:56:15Z |
publishDate | 2022-10-01 |
publisher | AIP Publishing LLC |
record_format | Article |
series | AIP Advances |
spelling | doaj.art-0cab8c584ca34226befd09e00b5b1c312022-12-22T03:36:05ZengAIP Publishing LLCAIP Advances2158-32262022-10-011210105319105319-810.1063/5.0014682Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasmaKashif Arshad0Stefaan Poedts1Alaa Dahshan2Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242, USACentre for Plasma Astrophysics, Celestijnenlaan 200B, 3001 Leuven, BelgiumDepartment of Physics, Faculty of Science, King Khalid University, 9004 Abha, Saudi ArabiaThe plasma modes are significantly influenced by the simple or/and molecular anions. The reciprocity of beam and tri-ion electron (TIE) plasmas is modeled by the kinetic theory. The set of Vlasov–Poisson equation is solved and decomposed by the Laguerre–Gaussian function under paraxial approximation. The beam plasma expedites unstable twisted modes (UTMs) in the TIE plasma. The UTM or instability is calibrated via axial and azimuthal wave numbers, wind speed, and its growth essence. The qualitative and quantitative anatomy of the instability threshold is also predicted. Our model is eminently applicable to the space plasmas and has been applied to the Ar+–F−–SF6− and Xe+–F−–SF6− electron plasmas, specifically.http://dx.doi.org/10.1063/5.0014682 |
spellingShingle | Kashif Arshad Stefaan Poedts Alaa Dahshan Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma AIP Advances |
title | Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma |
title_full | Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma |
title_fullStr | Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma |
title_full_unstemmed | Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma |
title_short | Quasi-electrostatic instability in non-gyrotropic tri-ion electron plasma |
title_sort | quasi electrostatic instability in non gyrotropic tri ion electron plasma |
url | http://dx.doi.org/10.1063/5.0014682 |
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