Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas
The beam-plasma particles distribution function is one of the parameters which plays an important role in the energy-traveling mechanism of the relativistic electrons generated by the laser-plasma interaction in the Inertial Confinement Fusion Plasma. This paper investigates an analytical expression...
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Damghan university
2024-03-01
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Series: | Iranian Journal of Astronomy and Astrophysics |
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Online Access: | https://ijaa.du.ac.ir/article_408_4545e3aa071195d0a12c7476305a2c54.pdf |
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author | Fatemeh Nejadtaghi Mohammad Mahdavi Saeid Hassan pour Hengameh Khanzadeh Ali Tavassoli |
author_facet | Fatemeh Nejadtaghi Mohammad Mahdavi Saeid Hassan pour Hengameh Khanzadeh Ali Tavassoli |
author_sort | Fatemeh Nejadtaghi |
collection | DOAJ |
description | The beam-plasma particles distribution function is one of the parameters which plays an important role in the energy-traveling mechanism of the relativistic electrons generated by the laser-plasma interaction in the Inertial Confinement Fusion Plasma. This paper investigates an analytical expression of the beam-plasma particles distribution function effect such as the Kappa, Semi-relativistic Maxwellian and bi-Maxwell distributions on the Weibel electromagnetic instability growth rate in strongly coupled plasmas under the low-frequency wave condition. The obtained results show that the maximum growth rate of the beam- plasma particles with semi-Maxwell distribution function is based on the temperature anisotropy parameter, density gradient, quantum and relativistic parameters has the highest possible value compared to the other two beam-plasma particles distribution functions. Also, the bi-Maxwellian distribution function has a more stable growth rate than the Kappa and the semi-Maxwell distribution functions. |
format | Article |
id | doaj-art-5a20e136bcf34a9cba8658a9b6883f4b |
institution | Kabale University |
issn | 2322-4924 2383-403X |
language | English |
publishDate | 2024-03-01 |
publisher | Damghan university |
record_format | Article |
series | Iranian Journal of Astronomy and Astrophysics |
spelling | doaj-art-5a20e136bcf34a9cba8658a9b6883f4b2025-01-12T10:03:29ZengDamghan universityIranian Journal of Astronomy and Astrophysics2322-49242383-403X2024-03-01111314410.22128/ijaa.2024.775.1177408Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled PlasmasFatemeh Nejadtaghi0Mohammad Mahdavi1Saeid Hassan pour2Hengameh Khanzadeh3Ali Tavassoli4Department of Physics, Faculty of Basic Sciences, Nour Branch, Islamic Azad University, Nour 4817935861, IranDepartment of Physics, Faculty of Basic Sciences, University of Mazandaran, P.O. Box 47415–416, Babolsar, IranDepartment of Physics, Faculty of Basic Sciences, Nour Branch, Islamic Azad University, Nour 4817935861, IranDepartment of Physics, Faculty of Basic Sciences, University of Mazandaran, P.O. Box 47415–416, Babolsar, IranDepartment of Physics, Faculty of Basic Sciences, Nour Branch, Islamic Azad University, Nour 4817935861, IranThe beam-plasma particles distribution function is one of the parameters which plays an important role in the energy-traveling mechanism of the relativistic electrons generated by the laser-plasma interaction in the Inertial Confinement Fusion Plasma. This paper investigates an analytical expression of the beam-plasma particles distribution function effect such as the Kappa, Semi-relativistic Maxwellian and bi-Maxwell distributions on the Weibel electromagnetic instability growth rate in strongly coupled plasmas under the low-frequency wave condition. The obtained results show that the maximum growth rate of the beam- plasma particles with semi-Maxwell distribution function is based on the temperature anisotropy parameter, density gradient, quantum and relativistic parameters has the highest possible value compared to the other two beam-plasma particles distribution functions. Also, the bi-Maxwellian distribution function has a more stable growth rate than the Kappa and the semi-Maxwell distribution functions.https://ijaa.du.ac.ir/article_408_4545e3aa071195d0a12c7476305a2c54.pdfweibel instabilitycoupled plasmastemperature anisotropybeam-plasma particles distribution functionlow-frequency wavestrongly coupled plasmas |
spellingShingle | Fatemeh Nejadtaghi Mohammad Mahdavi Saeid Hassan pour Hengameh Khanzadeh Ali Tavassoli Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas Iranian Journal of Astronomy and Astrophysics weibel instability coupled plasmas temperature anisotropy beam-plasma particles distribution function low-frequency wave strongly coupled plasmas |
title | Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas |
title_full | Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas |
title_fullStr | Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas |
title_full_unstemmed | Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas |
title_short | Analytical Expression of the Beam-Plasma Particles Distribution Function Effect on the Electromagnetic Instability Growth Rate in Strongly Coupled Plasmas |
title_sort | analytical expression of the beam plasma particles distribution function effect on the electromagnetic instability growth rate in strongly coupled plasmas |
topic | weibel instability coupled plasmas temperature anisotropy beam-plasma particles distribution function low-frequency wave strongly coupled plasmas |
url | https://ijaa.du.ac.ir/article_408_4545e3aa071195d0a12c7476305a2c54.pdf |
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