Arnold Diffusion, Quasi-ergodic Hypothesis, Instabilities for the Planar 3 Body Problem, and Central Configurations

阿诺德扩散、拟遍历假设、平面三体问题的不稳定性和中心配置

• 批准号: 1157830
• 负责人: Vadim Kaloshin
• 金额: $ 30万
• 依托单位: University of Maryland, College Park
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2011
• 资助国家: 美国
• 起止时间: 2011-08-16 至 2014-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1157830&HistoricalAwards=false
• 关键词: Arnold; Diffusion; Quasi; ergodic; Hypothesis

The intellectual merit of this proposal lies in developing techniques to understand formation of instabilities for abstract and concrete nearly integrable Hamiltonian systems. This includes the classical 3 body problem from celestial mechanics, which in particular describes the 3 body problem modeling the Sun-Jupiter-Asteroid system. So far mathematical description of instabilities for these and many other nearly integrable systems is limited. On the contrary stability for large measure of initial conditions is described by the famous KAM theory.The main goal of the project is analysis of the stability of motion of complex mechanical systems over long periods of time, focusing on the motion of planets. The behavior of such complex systems can be seen either as regular, as in the motion of planets, or chaotic, as in the motion of a hurricane. We shall analyze the interplay between regular and chaotic behavior to determine the length of stability of various systems, including the complicated three-body problem in classical mechanics, which involves determining the motion of three celestial bodies moving under no influence other than that of their mutual gravitation. Knowledge of instabilities of this system is fairly limited. The object is to develop techniques to investigate the stability time of these systems. The project will also involve graduate student training. Students will become expert celestial mechanics and will have first-hand experience in working on classical problems using relatively new mathematical tools.

这一建议的智力价值在于发展技术，以了解形成抽象和具体的近可积哈密顿系统的不稳定性。这包括天体力学中的经典三体问题，它特别描述了太阳-木星-小行星系统的三体问题。到目前为止，这些和许多其他几乎可积系统的不稳定性的数学描述是有限的。与此相反，著名的KAM理论描述了大尺度初始条件下的稳定性。该项目的主要目标是分析复杂机械系统长时间运动的稳定性，重点是行星的运动。这种复杂系统的行为可以被看作是规则的，如行星的运动，也可以被看作是混乱的，如飓风的运动。我们将分析规则和混沌行为之间的相互作用，以确定各种系统的稳定性长度，包括经典力学中复杂的三体问题，其中涉及确定三个天体在相互引力的影响下运动。关于这个系统的不稳定性的知识相当有限。我们的目标是开发技术来调查这些系统的稳定时间。该项目还将涉及研究生培训。学生将成为天体力学专家，并将有第一手的经验，在经典问题的工作使用相对较新的数学工具。