{"title":"约束玻色-爱因斯坦凝聚态涡旋的相对动力学","authors":"Tomoki Ohsawa","doi":"arxiv-2409.07657","DOIUrl":null,"url":null,"abstract":"We consider the relative dynamics -- the dynamics modulo rotational symmetry\nin this particular context -- of $N$ vortices in confined Bose--Einstein\nCondensates (BEC) using a finite-dimensional vortex approximation to the\ntwo-dimensional Gross--Pitaevskii equation. We give a Hamiltonian formulation\nof the relative dynamics by showing that it is an instance of the Lie--Poisson\nequation on the dual of a certain Lie algebra. Just as in our accompanying work\non vortex dynamics with the Euclidean symmetry, the relative dynamics possesses\na Casimir invariant and evolves in an invariant set, yielding an\nEnergy--Casimir-type stability condition. We consider three examples of\nrelative equilibria -- those solutions that are undergoing rigid rotations\nabout the origin -- with $N=2, 3, 4$, and investigate their stability using the\nstability condition.","PeriodicalId":501312,"journal":{"name":"arXiv - MATH - Mathematical Physics","volume":"22 3 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Relative Dynamics of Vortices in Confined Bose--Einstein Condensates\",\"authors\":\"Tomoki Ohsawa\",\"doi\":\"arxiv-2409.07657\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We consider the relative dynamics -- the dynamics modulo rotational symmetry\\nin this particular context -- of $N$ vortices in confined Bose--Einstein\\nCondensates (BEC) using a finite-dimensional vortex approximation to the\\ntwo-dimensional Gross--Pitaevskii equation. We give a Hamiltonian formulation\\nof the relative dynamics by showing that it is an instance of the Lie--Poisson\\nequation on the dual of a certain Lie algebra. Just as in our accompanying work\\non vortex dynamics with the Euclidean symmetry, the relative dynamics possesses\\na Casimir invariant and evolves in an invariant set, yielding an\\nEnergy--Casimir-type stability condition. We consider three examples of\\nrelative equilibria -- those solutions that are undergoing rigid rotations\\nabout the origin -- with $N=2, 3, 4$, and investigate their stability using the\\nstability condition.\",\"PeriodicalId\":501312,\"journal\":{\"name\":\"arXiv - MATH - Mathematical Physics\",\"volume\":\"22 3 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - MATH - Mathematical Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.07657\",\"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 - MATH - Mathematical Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.07657","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Relative Dynamics of Vortices in Confined Bose--Einstein Condensates
We consider the relative dynamics -- the dynamics modulo rotational symmetry
in this particular context -- of $N$ vortices in confined Bose--Einstein
Condensates (BEC) using a finite-dimensional vortex approximation to the
two-dimensional Gross--Pitaevskii equation. We give a Hamiltonian formulation
of the relative dynamics by showing that it is an instance of the Lie--Poisson
equation on the dual of a certain Lie algebra. Just as in our accompanying work
on vortex dynamics with the Euclidean symmetry, the relative dynamics possesses
a Casimir invariant and evolves in an invariant set, yielding an
Energy--Casimir-type stability condition. We consider three examples of
relative equilibria -- those solutions that are undergoing rigid rotations
about the origin -- with $N=2, 3, 4$, and investigate their stability using the
stability condition.