Comparative Analysis of Plasma Sheath Characteristics in One-Dimensional and Three-Dimensional Velocity Spaces Governing Nonextensive Electron Density

IF 1.3 4区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS
Oussama Jdaini, Abdelhak Missaoui, Mohamed El Bojaddaini, Morad El Kaouini, Hassan Chatei
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Abstract

In this study, we developed a model to explore the characteristics of a magnetized plasma sheath, containing positive ions, electrons, and neutral particles. The ions are described using a fluid model based on the continuity and momentum equations, while the electron distribution is analyzed using three cases: the Maxwell–Boltzmann distribution and the Tsallis distribution in both 1-D and 3-D velocity spaces. Applying the Sagdeev method, we established the modified Bohm sheath criterion to obtain the required ion velocity at the sheath entrance for all three cases. The lower Mach number limit for Bohm velocity modification depends on factors such as ion temperature, ionization frequency, collision frequency, magnetic field angle, nonextensive parameter q $$ q $$ , and the velocity space governing the density of nonextensive electrons, independent of magnetic field magnitude. Additionally, the electron velocity distribution was analyzed for various q-values, revealing that in 3-D velocity space, the energy range is broad and extensive, while in 1-D velocity spaces, it is narrower and confined within the broader 3-D interval. We examined the influence of key parameters on sheath characteristics under the Maxwellian distribution, as well as in 1-D and 3-D velocity spaces for the Tsallis distribution. The results demonstrated significant differences between the three cases, showing that in the 3-D case, the sheath thickness expands more compared to the 1-D and the Maxwell–Boltzmann distribution. This underscores the significance of accounting for the dimensionality of velocity space when investigating plasma sheath phenomena. Such understanding is crucial for optimizing plasma-surface interactions in various applications.

非扩展电子密度的一维和三维速度空间等离子体鞘层特性的比较分析
在这项研究中,我们开发了一个模型来探索磁化等离子体鞘层的特征,其中包含正离子、电子和中性粒子。用基于连续性和动量方程的流体模型描述离子,用麦克斯韦-玻尔兹曼分布和Tsallis分布三种情况分析电子在一维和三维速度空间中的分布。应用Sagdeev方法,建立了改进的Bohm鞘层判据,得到了三种情况下鞘层入口所需的离子速度。玻姆速度修正的马赫数下限取决于离子温度、电离频率、碰撞频率、磁场角度、非扩展参数q $$ q $$以及控制非扩展电子密度的速度空间等因素,与磁场大小无关。此外,对不同q值下的电子速度分布进行了分析,发现在三维速度空间中,能量范围较宽,而在一维速度空间中,能量范围较窄,限制在较宽的三维区间内。我们研究了麦克斯韦分布下关键参数对鞘层特性的影响,以及tallis分布下1-D和3-D速度空间的影响。结果显示了三种情况之间的显著差异,表明在三维情况下,鞘层厚度比一维和麦克斯韦-玻尔兹曼分布扩展得更大。这强调了在研究等离子体鞘层现象时考虑速度空间维度的重要性。这种理解对于在各种应用中优化等离子体表面相互作用是至关重要的。
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来源期刊
Contributions to Plasma Physics
Contributions to Plasma Physics 物理-物理:流体与等离子体
CiteScore
2.90
自引率
12.50%
发文量
110
审稿时长
4-8 weeks
期刊介绍: Aims and Scope of Contributions to Plasma Physics: Basic physics of low-temperature plasmas; Strongly correlated non-ideal plasmas; Dusty Plasmas; Plasma discharges - microplasmas, reactive, and atmospheric pressure plasmas; Plasma diagnostics; Plasma-surface interaction; Plasma technology; Plasma medicine.
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