等离子体中的尘埃离子声孤波与凯恩斯电子分布和离子的新经典分布

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
B. C. Kalita, R. Kalita, S. Das
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引用次数: 0

摘要

在这种带有负尘埃电荷、新经典分布的非热离子和凯恩斯分布电子的等离子体中,超音速和亚音速都只存在稀疏孤子。在不同温度值 α 下,超音速(M = 1.4)稀疏非活动孤子随着离子与尘埃密度比 Q 的增大而从小幅大幅凹增。在所有 M (>1) 条件下,稀有非活动孤子的振幅都呈凹形增长,但这种增长具有明显的特征。马赫数越小(如 M = 1.2),在整个 v0(离子漂移)范围内的孤子振幅就越小。在所有 r ( =ne0 /ni0 ) 条件下,稀疏超音速孤子的振幅随着非热参数 β 的增大而增大。该模型的动力学情景表明,等离子体中尘埃的质量应减少,以产生振幅更高的孤子。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Dust Ion Acoustic Solitary Waves in Plasma with Cairns Distributed Electrons and New Classical Distribution of Ions

In this composition of plasma with negative dust charge, new classical distribution of nonthermal ions and Cairns distributed electrons, both supersonic and subsonic only rarefactive solitons are found to exist. It appears to conclude that the solitons cease to exist at the increase of c. The supersonic (M = 1.4) rarefactive solitons considerably and concavely increase from small amplitude with the increase of the ion to dust density ratio Q for various values of temperature α . The concave but increasing growth of amplitude of the rarefactive solitons for all M (>1) exhibits its distinct character. Smaller the Mach number (e.g., for M = 1.2), smaller is the amplitude of the solitons throughout the range of v0 (ion drift). The amplitudes of the rarefactive supersonic solitons are found to increase at the increase of the nonthermal parameter β for all r ( =ne0 /ni0 ). The dynamical scenario of this model indicates that the mass of the dusts should decrease in the plasma to generate higher amplitude solitons.

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来源期刊
Astrophysics
Astrophysics 地学天文-天文与天体物理
CiteScore
0.90
自引率
20.00%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.
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