On dispersion and damping rates of dust-acoustic waves in hybrid non-thermal Vasyliunas–Cairns distributed plasmas

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Muhammad Ahsan Shahzad, Muhammad Sarfraz,  Aman-Ur-Rehman, Shahzad Mahmood, Muhammad Bilal, Hashim Farooq
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Abstract

The dispersion relation and Landau damping rate of dust-acoustic waves (DAWs) are studied by the incorporation of Poison–Vlasov model of the kinetic theory of plasmas. The real and imaginary frequencies of DAWs are obtained in a three-component plasma i.e., electrons, ions and dust grains. The electrons are taken as hybrid non-thermal Vasyliunas–Cairns distributed and in limiting cases as kappa and Cairns distributed as well, while the ions and dust are kept Maxwellian. The findings reveal that the simultaneous presence of two non-thermality parameters (i.e., \(\alpha \) and \(\kappa \)) have a remarkable impact on the dispersion and damping rates of DAWs as compared to the sole presence of any non-thermality parameter and also in the case of thermal electrons. It is also presented that the real and imaginary frequencies of DAWs are significantly influenced by the other important parameters, such as electron to ion temperature and density ratios. This work has notable significance in the understanding of important constituents of space plasmas i.e., thermal and non-thermal dusty plasmas in various environments of space plasmas, where the mixed particle distributions are observed.

Abstract Image

非热Vasyliunas-Cairns混合等离子体中尘埃-声波的色散和阻尼率
结合等离子体动力学理论中的Poison-Vlasov模型,研究了尘埃声波的色散关系和朗道阻尼率。在三组分等离子体中,即电子、离子和尘埃颗粒,获得了daw的实频率和虚频率。电子被认为是杂化的非热Vasyliunas-Cairns分布,在极限情况下也被认为是kappa和Cairns分布,而离子和尘埃则保持麦克斯韦分布。研究结果表明,与单独存在任何非热参数和热电子相比,同时存在两个非热参数(即\(\alpha \)和\(\kappa \))对DAWs的色散和阻尼率有显着的影响。结果还表明,电子离子温度和密度比等重要参数对daw的实、虚频率有显著影响。这项工作对于认识空间等离子体的重要组成部分,即热尘埃等离子体和非热尘埃等离子体在各种空间等离子体环境中的混合粒子分布具有重要意义。
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来源期刊
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy 地学天文-天文与天体物理
CiteScore
1.80
自引率
9.10%
发文量
84
审稿时长
>12 weeks
期刊介绍: The journal publishes original research papers on all aspects of astrophysics and astronomy, including instrumentation, laboratory astrophysics, and cosmology. Critical reviews of topical fields are also published. Articles submitted as letters will be considered.
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