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Propagation of Ion Solitary Pulses in Dense Astrophysical Electron-Positron-Ion Magnetoplasmas

机译:离子孤脉冲在密集天体电子正电子离子磁浆中的传播

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摘要

In this paper, we theoretically investigate the existence and propagation of low amplitude nonlinear ion waves in a dense plasma under the influence of a strong magnetic field. The plasma consists of ultra-relativistic and degenerate electrons and positrons and non-degenerate cold ions. Firstly, the appearance of two distinct linear modes and their evolution is studied by deriving a dispersion equation with the aid of Fourier analysis. Secondly, the dynamics of low amplitude ion solitary structures is investigated via a Korteweg-de Vries equation derived by employing a reductive perturbation method. The effects of various plasma parameters like positron concentration, strength of magnetic field, obliqueness of field, etc., are discussed in detail. At the end, analytical results are supplemented through numerical analysis by using typical representative parameters consistent with degenerate and ultra-relativistic magnetoplasmas of astrophysical regimes.
机译:在本文中,我们从理论上研究了在强磁场的影响下,低密度非线性离子波在密集等离子体中的存在和传播。等离子体由超相对论和简并的电子和正电子以及非简并的冷离子组成。首先,借助于傅立叶分析,通过推导色散方程,研究了两种不同线性模式的出现及其演化。其次,通过采用还原摄动法导出的Korteweg-de Vries方程,研究了低振幅离子孤立结构的动力学。详细讨论了各种等离子体参数的影响,例如正电子浓度,磁场强度,磁场倾斜度等。最后,通过使用与天体物理条件的简并和超相对论磁浆一致的典型代表参数,通过数值分析来补充分析结果。

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