{"title":"Numerical Study of Polytropes with n = 1 and Differential Rotation","authors":"T. L. Razinkova, A. V. Yudin, S. I. Blinnikov","doi":"10.1134/S1063772925701367","DOIUrl":null,"url":null,"abstract":"<p>The solution space of differentially rotating polytropes with <span>\\(n = 1\\)</span> 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, <span>\\(\\sigma \\simeq 2\\)</span>. 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 <span>\\(\\tau \\)</span>, which has raised the question of their stability with respect to fragmentation.</p>","PeriodicalId":55440,"journal":{"name":"Astronomy Reports","volume":"68 12","pages":"1423 - 1436"},"PeriodicalIF":1.1000,"publicationDate":"2025-03-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy Reports","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S1063772925701367","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
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.
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.