Numerical Study of Polytropes with n = 1 and Differential Rotation

IF 0.7 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Reports Pub Date : 2025-03-14 DOI:10.1134/S1063772925701367
T. L. Razinkova, A. V. Yudin, S. I. Blinnikov
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Abstract

The solution space of differentially rotating polytropes with \(n = 1\) has been studied numerically. The existence of three different types of configurations: from spheroids to thick tori, hockey puck-like bodies and spheroids surrounded by a torus, separate from or merging with the central body has been proved. It has been shown that the last two types appear only at moderate degrees of rotation differentiality, \(\sigma \simeq 2\). Rigid-body or weakly differential rotation, as well as strongly differential, have not led to any “exotic” types of configurations. Many calculated configurations have had extremely large values of parameter \(\tau \), which has raised the question of their stability with respect to fragmentation.

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n = 1和微分旋转多多体的数值研究
对具有(n = 1)的微分旋转多面体的解空间进行了数值研究。证明了存在三种不同类型的构型:从球体到厚环体、冰球状体和被环体包围的球体,它们与中心体分离或合并。研究表明,后两种类型只出现在中等旋转差度的情况下,即 \(\sigma \simeq 2\).刚体或弱微分旋转以及强微分旋转并没有导致任何 "奇特 "类型的构型。许多计算出的构型的参数值都非常大,这就提出了它们在碎裂方面的稳定性问题。
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来源期刊
Astronomy Reports
Astronomy Reports 地学天文-天文与天体物理
CiteScore
1.40
自引率
20.00%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.
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