dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorMuriano, A. G R
dc.creatorDa Silva, M. F A
dc.date2014-05-27T11:18:15Z
dc.date2016-10-25T18:14:34Z
dc.date2014-05-27T11:18:15Z
dc.date2016-10-25T18:14:34Z
dc.date1997-09-01
dc.date.accessioned2017-04-06T00:50:04Z
dc.date.available2017-04-06T00:50:04Z
dc.identifierAmerican Journal of Physics, v. 65, n. 9, p. 914-917, 1997.
dc.identifier0002-9505
dc.identifierhttp://hdl.handle.net/11449/65171
dc.identifierhttp://acervodigital.unesp.br/handle/11449/65171
dc.identifier10.1119/1.18682
dc.identifierWOS:A1997XU38600018
dc.identifier2-s2.0-0031508615.pdf
dc.identifier2-s2.0-0031508615
dc.identifierhttp://dx.doi.org/10.1119/1.18682
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/886921
dc.descriptionThe magnetostatic field of an infinite rectilinear current placed in the stationary gravitational field of a rotating cosmic string is found. An interesting aspect of this problem is that although the metric is mathematically very simple, its physical meaning is not trivial. It depends only on topological parameters. So, the cosmic string vacuum space-time is locally equivalent to the Minkowski space-time, but not globally. The calculations are so simple that they can easily be shown in the classroom. © 1997 American Association of Physics Teachers.
dc.languageeng
dc.relationAmerican Journal of Physics
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.titleThe magnetic field of a current carrying cosmic string
dc.typeOtro


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