SPINNING STRINGS AS TORSION LINE SPACETIME DEFECTS

dc.creatorLETELIER, PS
dc.date1995
dc.dateFEB
dc.date2014-12-16T11:35:15Z
dc.date2015-11-26T18:04:22Z
dc.date2014-12-16T11:35:15Z
dc.date2015-11-26T18:04:22Z
dc.date.accessioned2018-03-29T00:46:28Z
dc.date.available2018-03-29T00:46:28Z
dc.identifierClassical And Quantum Gravity. Iop Publishing Ltd, v. 12, n. 2, n. 471, n. 478, 1995.
dc.identifier0264-9381
dc.identifierWOS:A1995QN27600016
dc.identifier10.1088/0264-9381/12/2/016
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/74392
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/74392
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/74392
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1292826
dc.descriptionA consistent description of spinning strings with dislocations (chiral strings) as a missing part of the spacetime manifold (spacetime defect) is achieved by introducing a line of torsion along the string. Also, the definition of a spin-dislocation tenser associated with the chiral string allows its interpretation in the context of the Einstein-Cartan theory of gravitation. Some generalizations, as well as the Dirac equations, are briefly discussed. In particular, we argue that the behaviour of the fermions near the chiral string can be used to test the torsion hypothesis.
dc.description12
dc.description2
dc.description471
dc.description478
dc.languageen
dc.publisherIop Publishing Ltd
dc.publisherBristol
dc.publisherInglaterra
dc.relationClassical And Quantum Gravity
dc.relationClass. Quantum Gravity
dc.rightsfechado
dc.rightshttp://iopscience.iop.org/page/copyright
dc.sourceWeb of Science
dc.subjectCosmic Strings
dc.subjectTopological Defects
dc.titleSPINNING STRINGS AS TORSION LINE SPACETIME DEFECTS
dc.typeArtículos de revistas


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