Perturbed R3BP with Logarithmic Potential

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Abdullah, S. K. Sahdev
{"title":"Perturbed R3BP with Logarithmic Potential","authors":"Abdullah,&nbsp;S. K. Sahdev","doi":"10.1134/S1063772923340012","DOIUrl":null,"url":null,"abstract":"<p>This paper investigates the dynamical behavior of the effects of perturbations on the motion of infinitesimal body in the restricted three-body problem (R3BP) with logarithmic potential where both spherical primaries are taken as source of radiation pressure and third infinitesimal body is considered as variable mass according to Jeans law. We also have taken the effects of coriolis and centrifugal forces. For further investigations, we derive the equations of motion of the infinitesimal body where we get the effective variation due to parameters. Furthermore, we numerically illustrate some analysis of potential function, the locations of equilibrium points, trajectories allocations, surfaces of section, regions of motion and basins of attraction. Finally, the stability examination is done for the equilibrium points using Meshcherskii space-time inverse transformations.</p>","PeriodicalId":55440,"journal":{"name":"Astronomy Reports","volume":"67 12","pages":"1473 - 1482"},"PeriodicalIF":1.1000,"publicationDate":"2024-02-25","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/S1063772923340012","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

This paper investigates the dynamical behavior of the effects of perturbations on the motion of infinitesimal body in the restricted three-body problem (R3BP) with logarithmic potential where both spherical primaries are taken as source of radiation pressure and third infinitesimal body is considered as variable mass according to Jeans law. We also have taken the effects of coriolis and centrifugal forces. For further investigations, we derive the equations of motion of the infinitesimal body where we get the effective variation due to parameters. Furthermore, we numerically illustrate some analysis of potential function, the locations of equilibrium points, trajectories allocations, surfaces of section, regions of motion and basins of attraction. Finally, the stability examination is done for the equilibrium points using Meshcherskii space-time inverse transformations.

Abstract Image

具有对数电位的扰动 R3BP
摘要 本文研究了在具有对数势能的受限三体问题(R3BP)中,扰动对无穷小体运动影响的动力学行为,在该问题中,两个球形基体都被视为辐射压力源,而第三个无穷小体则被视为根据让斯定律的可变质量。我们还考虑了科里奥利力和离心力的影响。为了进一步研究,我们推导出了无穷小体的运动方程,其中我们得到了参数引起的有效变化。此外,我们用数值说明了势函数、平衡点位置、轨迹分配、截面、运动区域和吸引盆地的一些分析。最后,我们利用 Meshcherskii 时空反变换对平衡点进行了稳定性检验。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
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.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信