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Compressive and rarefactive dust ion-acoustic solitary waves with degenerate electron-positron-ion plasma

机译:简并电子正电子离子等离子体的压缩和稀疏粉尘离子声孤立波

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摘要

The nonlinear propagation of dust ion-acoustic (DIA) waves in a unmagnetized collisionless degenerate dense plasma (containing degenerate electron and positron, and classical ion fluids) has been theoretically investigated. The K-dV equation has been derived by employing the reductive perturbation method and by taking into account the effect of different plasma parameters in plasma fluid. The stationary solitary wave solution of K-dV equation is obtained, and numerically analyzed to identify the basic properties of DIA solitary structures. It has been shown that depending on plasma parametric values, the degenerate plasma under consideration supports compressive or rarefactive solitary structures. It has been also found that the effect of pressures on electrons, ions, and positrons significantly modify the basic features of solitary waves that are found to exist in such a plasma system. The relevance of our results in astrophysical objects such as white dwarfs and neutron stars, which are of scientific interest, is discussed briefly.
机译:从理论上研究了未磁化的无碰撞简并稠密等离子体(包含简并电子和正电子以及经典离子流体)中尘埃离子声波(DIA)的非线性传播。 K-dV方程是通过采用还原扰动方法并考虑到血浆流体中不同血浆参数的影响而得出的。得到了K-dV方程的孤立孤波解,并对其进行了数值分析,以确定DIA孤立结构的基本性质。已经显示出,取决于等离子体参数值,所考虑的简并等离子体支持压缩或稀疏的孤立结构。还已经发现,压力对电子,离子和正电子的影响极大地改变了在这种等离子体系统中发现的孤立波的基本特征。简要讨论了我们的研究结果与天体物理物体(如白矮星和中子星)的相关性,这些天体具有科学意义。

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