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Ion-acoustic compressive and rarefactive solitary waves in unmagnetised plasmas with positrons and two-temperature superthermal electrons

机译:离子声压缩且稀有的孤立在具有正弦和两温超热电子的未磁化等离子体中的孤立波

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Ion-acoustic solitary waves (IASWs) in plasma consisting of ions, positrons and superthermal electrons in two distinct temperatures have been studied. The reductive perturbation method (RPM) has been employed to derive the Kortewega??de Vries and modified KdV equation. Numerical and analytical studies show that compressive and rarefactive solitons exist for the selected parametric range depending on the spectral indexes, $?o (?o_{h},?o_{c})$ and their respective densities ($u,mu$). It is found that spectral indexes ($?o_{h},?o_{c}$) and their relative densities have significant impact on the basic properties, i.e., amplitude and width as well as on the nature of IASWs. Variations of amplitude and width for the compressive and rarefactive solitary waves have been analysed graphically with different plasma parameters like spectral indexes of cold and hot electrons ($k_{c}, k_{h}$), their respective densities, ionic temperature ratio, positron temperature ratio as well as with the temperature ratio of the two-electron species. The amplitude of the compressive (rarefactive) solitary waves increases (decreases) on increasing $k_{h}$. However, the amplitude of the compressive (rarefactive) solitary waves decreases (increases) on increasing $k_{c}$. The investigations of such solitary waves may be helpful for the critical understanding of space where superthermal electrons with two different temperatures exist along with positrons and ions (e.g. Saturna??s magnetosphere, pulsar magnetosphere).
机译:已经研究了由离子,正源和高温电子组成的等离子体中的离子声学孤波(IASW)已经研究过两种不同的温度。已经采用了还原性扰动方法(RPM)来导出Kortewega?De VRIES和修改的KDV方程。数值和分析研究表明,根据光谱索引,$ΔO(?O_ {h} ,? O_ {c})$及其各自的密度($ nu, mu $)。发现光谱索引($?O_ {H} ,? O_ {C} $)和它们的相对密度对基本属性具有显着影响,即幅度和宽度以及IASW的性质。用不同的等离子体参数以不同的等离子体参数(如冷热电子的光谱索引($ k_ {c},k_ {h} $),它们各自的密度,离子温度比为不同的等离子体参数来分析压缩和稀疏孤立波的幅度和宽度的变化。正电子温度比以及两种电子物种的温度比。压缩(磁解)孤波的幅度增加(减少)增加$ k_ {h} $。然而,压缩(磁解)孤波的幅度降低(增加)上增加$ k_ {c} $。这种孤波的调查可能有助于对具有两个不同温度的超高热电子存在的空间的批判性理解以及正弦和离子(例如Saturna'On磁层,脉冲磁层)。

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