Equilibrium and stability in Robe’s restricted problem with a line segment and modified potential

IF 2.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Sumit Kumar, Bhavneet Kaur, Mukesh Kumar, Nitesh Kumar
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Abstract

In mathematics, particularly in dynamical systems theory, equilibrium points and their stability are of critical importance, as they represent the steady-state solutions of a system. This study examines the equilibrium points and their stability in a modified formulation of a well known dynamical system: the Robe’s problem. Unlike the original Robe problem where the primary \(m_{2}\) is treated as a point mass, we have modeled \(m_{2}\) as a line segment. The line segment is assumed to produce modified Newtonian potential instead of classical Newtonian potential. The introduction of a modified Newtonian potential leads to substantial changes in the system’s dynamics when compared to the classical Robe’s problem with line segment. Using analytical techniques, we show that the modified system admits only a single collinear equilibrium point, in contrast to the classical case, which allows infinite equilibrium points, including non-collinear (degenerate equilibrium set) and out-of-plane equilibrium points. A linear stability analysis of this equilibrium point indicates marginal stability, with all eigenvalues lying purely on the imaginary axis. This suggests that small perturbations neither grow exponentially nor decay, indicating the absence of inherent damping or restoring mechanisms. Overall, the findings highlight how departures from point-mass assumptions and classical Newtonian potentials can significantly influence the qualitative dynamics of Robe’s restricted three-body system by breaking the degeneracy of equilibrium configuration.

Abstract Image

具有线段和修正势的罗布受限问题的平衡与稳定性
在数学中,特别是在动力系统理论中,平衡点及其稳定性是至关重要的,因为它们代表了系统的稳态解。本研究考察了一个著名动力系统的修正公式中的平衡点及其稳定性:罗布问题。与原始的Robe问题不同,原始的\(m_{2}\)被视为一个质点,我们将\(m_{2}\)建模为一个线段。假设线段产生修正的牛顿势而不是经典的牛顿势。与经典的罗布线段问题相比,引入改进的牛顿势导致系统动力学发生了实质性变化。利用解析技术,我们证明了改进后的系统只允许一个共线平衡点,而不是经典情况下允许无限个平衡点,包括非共线(退化平衡集)和面外平衡点。该平衡点的线性稳定性分析表明,所有的特征值都完全位于虚轴上,从而具有边际稳定性。这表明小的扰动既不呈指数增长也不衰减,表明缺乏固有的阻尼或恢复机制。总的来说,这些发现强调了偏离点质量假设和经典牛顿势如何通过打破平衡构型的简并来显著影响罗布受限三体系统的定性动力学。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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