Please use this identifier to cite or link to this item: https://doi.org/10.3934/dcdss.2020067
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dc.titleAlmost all 3-body relative equilibria on S2 and H2 are inclined
dc.contributor.authorDiacu, F.
dc.contributor.authorZhu, S.
dc.date.accessioned2021-12-06T04:27:21Z
dc.date.available2021-12-06T04:27:21Z
dc.date.issued2019
dc.identifier.citationDiacu, F., Zhu, S. (2019). Almost all 3-body relative equilibria on S2 and H2 are inclined. Discrete and Continuous Dynamical Systems - Series S 13 (4) : 1131-1143. ScholarBank@NUS Repository. https://doi.org/10.3934/dcdss.2020067
dc.identifier.issn1937-1632
dc.identifier.urihttps://scholarbank.nus.edu.sg/handle/10635/209615
dc.description.abstractWe answer here a question posed by F. Diacu in 2012 that asked whether there exist relative equilibria on S2 and H2 that move in a plane non-perpendicular to the rotation axis. For 3-body non-geodesic ordinary central configurations on S2 and H2, we find all relative equilibria that move in a plane perpendicular to the rotation axis. We also show that the set of shapes of 3-body non-geodesic ordinary central configurations on S2 and H2 is a 3-dimensional manifold. Then we conclude that almost all 3-body relative equilibria move in planes non-perpendicular to the rotation axis. © 2019 American Institute of Mathematical Sciences. All rights reserved.
dc.publisherAmerican Institute of Mathematical Sciences
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.sourceScopus OA2019
dc.subjectCelestial mechanics
dc.subjectCentral configurations
dc.subjectCurved 3-body problem
dc.subjectRelative equilibria
dc.subjectThree-body problem
dc.typeArticle
dc.contributor.departmentYALE-NUS COLLEGE
dc.description.doi10.3934/dcdss.2020067
dc.description.sourcetitleDiscrete and Continuous Dynamical Systems - Series S
dc.description.volume13
dc.description.issue4
dc.description.page1131-1143
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