{"title":"具有随时间变化的世俗扰动的拉格朗日行星方程","authors":"Barnabás Deme","doi":"arxiv-2405.18140","DOIUrl":null,"url":null,"abstract":"The long-term evolution of astrophysical systems is driven by a Hamiltonian\nthat is independent of the fast angle. As this Hamiltonian may contain\nexplicitly time-dependent parameters, the conservation of mechanical energy is\nnot guaranteed in such systems. We derive how the semi-major axis evolves in\nthese cases. We analyze two astrophysically interesting examples, those of the\nharmonic and quadrupole perturbations.","PeriodicalId":501482,"journal":{"name":"arXiv - PHYS - Classical Physics","volume":"34 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-05-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Lagrange's planetary equations with time-dependent secular perturbations\",\"authors\":\"Barnabás Deme\",\"doi\":\"arxiv-2405.18140\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The long-term evolution of astrophysical systems is driven by a Hamiltonian\\nthat is independent of the fast angle. As this Hamiltonian may contain\\nexplicitly time-dependent parameters, the conservation of mechanical energy is\\nnot guaranteed in such systems. We derive how the semi-major axis evolves in\\nthese cases. We analyze two astrophysically interesting examples, those of the\\nharmonic and quadrupole perturbations.\",\"PeriodicalId\":501482,\"journal\":{\"name\":\"arXiv - PHYS - Classical Physics\",\"volume\":\"34 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-05-28\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Classical Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2405.18140\",\"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 - Classical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2405.18140","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Lagrange's planetary equations with time-dependent secular perturbations
The long-term evolution of astrophysical systems is driven by a Hamiltonian
that is independent of the fast angle. As this Hamiltonian may contain
explicitly time-dependent parameters, the conservation of mechanical energy is
not guaranteed in such systems. We derive how the semi-major axis evolves in
these cases. We analyze two astrophysically interesting examples, those of the
harmonic and quadrupole perturbations.