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arXiv 2303.13640physics.plasm-phastro-ph.GA
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实验室与天体物理尘埃等离子体中由阻力和静电相互作用介导的共振不稳定性

Resonant instabilities mediated by drag and electrostatic interactions in laboratory and astrophysical dusty plasmas

Ben Y. Israeli, Amitava Bhattacharjee, Hong Qin

AI总结:

本文将共振阻力不稳定性中的缺陷特征值共振机制推广为共振不稳定性框架,揭示双流、丝状电离与声学RDI的物理共性及其实验室研究价值。

摘要:

众所周知,尘埃等离子体可支持多种多样的不稳定性,既包括标准等离子体不稳定性的推广形式,也包括由尘埃系统特有效应引起的不稳定性。近期研究表明,一类被称为共振阻力不稳定性(RDIs)的新型、广泛的流动不稳定性,可归因于一种特殊的共振现象,该现象表现为线性化尘埃/流体系统的缺陷特征值。本文证明,这种共振现象并非RDIs所独有,并可作为理解更广泛的一类不稳定性(称为共振不稳定性)的框架。研究特别关注实验室尘埃等离子体中观察到的丝状电离不稳定性以及双流不稳定性。结果表明,由于尘埃-离子声双流不稳定性与声学RDI在基础物理上具有共性,这些不稳定性应在天体物理尘埃等离子体中高度重叠的参数区间内具有相关性。本文提出,这些模式(以及丝状不稳定性)在实验可实现性上的类似重叠,使在实验室中对复杂且与天体物理相关的不稳定性动力学进行实验研究成为可能。

英文摘要:

Dusty plasmas are known to support a diverse range of instabilities, including both generalizations of standard plasma instabilities and ones caused by effects specific to dusty systems. It has been recently demonstrated that a novel broad class of streaming instabilities, termed resonant drag instabilities (RDIs), can be attributed to a particular resonance phenomenon, manifested by defective eigenvalues of the linearized dust/fluid system. In this work, it is demonstrated that this resonance phenomenon is not unique to RDIs and can be used as a framework to understand a wider range of instabilities, termed resonant instabilities. Particular attention is given to the filamentary ionization instability seen in laboratory dusty plasmas and to the two-stream instability. It is shown that, due to the commonalities in underlying physics between the dust-ion-acoustic two-stream instability and the acoustic RDI, these instabilities should be relevant in strongly overlapping regimes in astrophysical dusty plasmas. It is proposed that a similar overlap in the experimental accessibility of these modes (and of the filamentary instability) allows for the possibility of experimental investigation in the laboratory of complex and astrophysically relevant instability dynamics.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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