研究了限制三体构型中非共线振动点在非均质有限直段条件下的非线性稳定性

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Solar System Research Pub Date : 2023-07-04 DOI:10.1134/S0038094623030024
Bhawna Singh, Kumari Shalini, Sada Nand Prasad, Abdullah A. Ansari
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引用次数: 0

摘要

本文的研究重点是分析限制三体问题(R3BP)中三角形平衡点\({{\mathcal{L}}_{4}}\)和\({{\mathcal{L}}_{5}}\)的非线性稳定性。在非均质初级和辐射有限直段次级的影响下,以及在科里奥利力和离心力的作用下,找到了稳定的条件。这项研究是通过对哈密顿量进行归一化,以得到哈密顿量的Birkhoff标准形式来完成的,因为哈密顿量的标准形式对于研究平衡点的非线性稳定性很重要。在存在共振情况\(\omega _{1}^{'} = 2\omega _{2}^{'}\)和\(\omega _{1}^{'} = 3\omega _{2}^{'}\)的情况下,对KAM定理的条件进行了检验,发现对于三种质量比值\({{\mu }_{1}},\)\({{\mu }_{2}}\)和\({{\mu }_{3}}.\),这些条件都不成立。\({{\mathcal{L}}_{4}}\)和\({{\mathcal{L}}_{5}}\)在线性稳定范围内是非线性稳定的\(0 < \mu < {{\mu }_{c}},\),其中\({{\mu }_{c}}\)为质量参数的临界值\(\mu .\)因此,在存在上述扰动的情况下,三角形平衡点对于这三个质量比值是不稳定的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Study the Non-Linear Stability of Non-Collinear Libration Point in the Restricted Three-Body Configuration When the Shapes of the Primaries are Taken as Heterogeneous and Finite-Straight Segment

The main focus of the present research work is to analyze the non-linear stability of the triangular equilibrium points \({{\mathcal{L}}_{4}}\) and \({{\mathcal{L}}_{5}}\) in the restricted three-body problem (R3BP). The condition of stability has been found out under the influence of the heterogeneous primary and a radiating finite-straight segment secondary and also under the effect by Coriolis as well as Centrifugal forces. This piece of research has been done by doing the normalization of the Hamiltonian in order to attained the Birkhoff’s normal form of the Hamiltonian, since normal forms of Hamiltonian are important to study the non-linear stability of equilibrium points. The conditions of KAM Theorem have been examined in the presence of resonance cases \(\omega _{1}^{'} = 2\omega _{2}^{'}\) and \(\omega _{1}^{'} = 3\omega _{2}^{'}\) and found that these conditions have been failed for three values of mass ratios \({{\mu }_{1}},\) \({{\mu }_{2}}\) and \({{\mu }_{3}}.\) Except these three values, \({{\mathcal{L}}_{4}}\) and \({{\mathcal{L}}_{5}}\) are stable in non-linear sense within the range of linear stability \(0 < \mu < {{\mu }_{c}},\) where \({{\mu }_{c}}\) is the critical value of mass parameter \(\mu .\) Consequently, in the presence of above mentioned purturbations the triangular equilibrium points are unstable for these three values of mass ratios.

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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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