非扩展Tsallis动力学中考虑磁场和辐射的原行星盘的Jeans不稳定性

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
A. V. Kolesnichenko
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引用次数: 0

摘要

在非扩展Tsallis统计的框架下,我们导出了由导电理想q气体和修正辐射光子气体混合组成的自引力原行星盘的Jeans引力不稳定性判据。不稳定性判据由盘中性物质和磁化等离子体在修正黑体辐射下的色散关系导出。基于依赖于变形参数的非扩展Tsallis量子熵,我们构造了光子气体的热力学。研究表明,黑体q辐射可以稳定纯气态圆盘的非扩散介质的状态,而对于导电圆盘,磁场和辐射压力只在扰动波的横传播模式下改变了Jeans不稳定判据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Jeans’ Instability of a Protoplanetary Disk with Accounting for the Magnetic Field and Radiation Modified within the Nonextensive Tsallis Kinetics

In the framework of nonextensive Tsallis statistics, we derive the Jeans gravitational instability criteria for a self-gravitating protoplanetary disk, the matter of which consists of a mixture of a conducting ideal q-gas and modified radiation of a photon gas. The instability criteria are derived from the corresponding dispersion relations written for both neutral matter of the disk and magnetized plasma with modified blackbody radiation. We construct the thermodynamics of a photon gas based on the nonextensive Tsallis quantum entropy that depends on the deformation parameter. It has been shown that the blackbody q-radiation can stabilize the state of a nonextensive medium of a purely gaseous disk, while for an electrically conducting disk, the Jeans instability criterion is modified by the magnetic field and radiation pressure only in the transverse mode of propagation of a perturbation wave.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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