{"title":"Equilibrium and stability in Robe’s restricted problem with a line segment and modified potential","authors":"Sumit Kumar, Bhavneet Kaur, Mukesh Kumar, Nitesh Kumar","doi":"10.1007/s10509-026-04584-2","DOIUrl":null,"url":null,"abstract":"<div><p>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 <span>\\(m_{2}\\)</span> is treated as a point mass, we have modeled <span>\\(m_{2}\\)</span> 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.</p></div>","PeriodicalId":8644,"journal":{"name":"Astrophysics and Space Science","volume":"371 5","pages":""},"PeriodicalIF":2.1000,"publicationDate":"2026-05-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysics and Space Science","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10509-026-04584-2","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
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.
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.
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