{"title":"受限三体问题中作为拉普拉斯微扰理论结果的马修方程","authors":"Alexey Rosaev, Eva Plavalova","doi":"arxiv-2408.04298","DOIUrl":null,"url":null,"abstract":"Linear equations with periodic coefficients describe the behavior of various\ndynamical systems. This studying is devoted to their applications to the\nplanetary restricted three-body problem (RTBP). Here we consider the Laplace\nmethod for determining perturbation in coordinates. We show that classical\ntheory of perturbation leads to a linear equation with periodic coefficients.\nThan we present a modification of Laplace method. This modification allows us\nto study motion over a longer time interval.","PeriodicalId":501209,"journal":{"name":"arXiv - PHYS - Earth and Planetary Astrophysics","volume":"192 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Mathieu equation as a result of Laplace perturbation theory in the restricted three body problem\",\"authors\":\"Alexey Rosaev, Eva Plavalova\",\"doi\":\"arxiv-2408.04298\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Linear equations with periodic coefficients describe the behavior of various\\ndynamical systems. This studying is devoted to their applications to the\\nplanetary restricted three-body problem (RTBP). Here we consider the Laplace\\nmethod for determining perturbation in coordinates. We show that classical\\ntheory of perturbation leads to a linear equation with periodic coefficients.\\nThan we present a modification of Laplace method. This modification allows us\\nto study motion over a longer time interval.\",\"PeriodicalId\":501209,\"journal\":{\"name\":\"arXiv - PHYS - Earth and Planetary Astrophysics\",\"volume\":\"192 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-08-08\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Earth and Planetary Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2408.04298\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Earth and Planetary Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.04298","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Mathieu equation as a result of Laplace perturbation theory in the restricted three body problem
Linear equations with periodic coefficients describe the behavior of various
dynamical systems. This studying is devoted to their applications to the
planetary restricted three-body problem (RTBP). Here we consider the Laplace
method for determining perturbation in coordinates. We show that classical
theory of perturbation leads to a linear equation with periodic coefficients.
Than we present a modification of Laplace method. This modification allows us
to study motion over a longer time interval.