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dc.contributor.authorHerrera, Jónatan
dc.contributor.authorRosa, M. de la
dc.contributor.authorRubio, Rafael
dc.date.accessioned2021-09-07T09:41:54Z
dc.date.available2021-09-07T09:41:54Z
dc.date.issued2021
dc.identifier.urihttp://hdl.handle.net/10396/21559
dc.description.abstractIn this paper, we analyze trajectories of spacelike curves that are critical points of a Lagrangian depending on its total torsion. We focus on two important families of spacetimes, generalized Robertson–Walker and standard static spacetimes. For the former, we show that such trajectories are those with a constant curvature. For the latter, we also obtain a characterization in terms of the curvature of the trajectory but in this case measured with an appropriate conformal metric.es_ES
dc.format.mimetypeapplication/pdfes_ES
dc.language.isoenges_ES
dc.publisherAmerican Institute of Physicses_ES
dc.rightshttps://creativecommons.org/licenses/by-nc-nd/4.0/es_ES
dc.sourceJournal of Mathematical Physics 62, 10.1063/5.0041384 (2021)es_ES
dc.subjectSpacelike curveses_ES
dc.subjectStationary spacetimees_ES
dc.subjectLagrangianses_ES
dc.subjectRelativistic particleses_ES
dc.subjectGeodesic trajectoryes_ES
dc.titleRelativistic particles with torsion in three-dimensional non-vacuum spacetimeses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherversionhttps://doi.org/10.1063/5.0041384es_ES
dc.relation.projectIDGobierno de España. MTM2016-78807-C2-2-Pes_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


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