Chaos and Taub-NUT related spacetimes

dc.creatorLetelier, PS
dc.creatorVieira, WM
dc.date1998
dc.date46569
dc.date2014-12-02T16:26:15Z
dc.date2015-11-26T17:27:41Z
dc.date2014-12-02T16:26:15Z
dc.date2015-11-26T17:27:41Z
dc.date.accessioned2018-03-29T00:14:50Z
dc.date.available2018-03-29T00:14:50Z
dc.identifierPhysics Letters A. Elsevier Science Bv, v. 244, n. 5, n. 324, n. 328, 1998.
dc.identifier0375-9601
dc.identifierWOS:000075040600003
dc.identifier10.1016/S0375-9601(98)00363-6
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/62723
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/62723
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/62723
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1284861
dc.descriptionThe occurrence of chaos for test particles moving in a Taub-NUT spacetime with a dipolar halo perturbation is studied using Poincare sections. We find that the NUT parameter (magnetic mass) attenuates the presence of chaos. (C) 1998 Elsevier Science B.V.
dc.description244
dc.description5
dc.description324
dc.description328
dc.languageen
dc.publisherElsevier Science Bv
dc.publisherAmsterdam
dc.publisherHolanda
dc.relationPhysics Letters A
dc.relationPhys. Lett. A
dc.rightsfechado
dc.rightshttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dc.sourceWeb of Science
dc.subjectBlack-hole
dc.subjectPerturbation
dc.subjectSymmetry
dc.titleChaos and Taub-NUT related spacetimes
dc.typeArtículos de revistas


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