Kumari Ranjana , M. Shahbaz Ullah , M. Javed Idrisi
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引用次数: 0
Abstract
This manuscript delves into the exploration of the existence and uniqueness of the th level approximation within the context of the inertial restricted three-body problem. In this scenario, two massive celestial bodies, namely Earth and the Sun, are held stationary along a straight line, while a less massive object serves as an artificial satellite. Within the manuscript, we have uncovered solutions expressed in terms of quadratures, infinite series, and transcendental functions. Our investigation employs a system of integral equations to address the challenge posed by these two immobile centers. The process initiates with the derivation of the equations of motion for the Earth, Sun, and satellite system, all considered within the inertial coordinate system. Subsequently, we formulate the th level approximation and present its solution for the linear integral equations system. We also meticulously determine the conditions necessary for the solution to converge. Additionally, we engage in an in-depth discussion regarding the existence of such a solution. Moreover, the manuscript firmly establishes the uniqueness of this solution, assuring its singularity. Furthermore, we undertake a rigorous analysis to quantify the error associated with the th level approximated solution.
本手稿以惯性受限三体问题为背景,深入探讨 nth 级近似的存在性和唯一性。在这种情况下,两个大质量天体(即地球和太阳)沿直线静止不动,而一个质量较小的天体充当人造卫星。在手稿中,我们发现了用二次函数、无穷级数和超越函数表示的解。我们的研究采用了一个积分方程组来解决这两个不动中心带来的挑战。我们首先推导出地球、太阳和卫星系统的运动方程,所有方程都在惯性坐标系中进行考虑。随后,我们提出了第 n 级近似,并给出了线性积分方程系统的解法。我们还细致地确定了求解收敛的必要条件。此外,我们还深入讨论了这种解的存在性。此外,手稿还牢固确立了该解法的唯一性,确保其奇异性。此外,我们还进行了严格的分析,以量化与第 n 级近似解相关的误差。
Astronomy and ComputingASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍:
Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.