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Vacuum polarization by a magnetic flux in a cosmic string background.

dc.contributor.authorSpinelly, J.
dc.contributor.authorMello, ERB de
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniv Fed Paraiba
dc.date.accessioned2015-03-18T15:53:43Z
dc.date.available2015-03-18T15:53:43Z
dc.date.issued2004-02-01
dc.description.abstractIn this paper we analyse the vacuum polarization effects due to a magnetic flux on massless fermionic fields in a cosmic string background. Three distinct configurations of magnetic fields are considered. In all of them the magnetic fluxes are confined in a long cylindrical tube of finite radius.en
dc.description.affiliationUniv Estadual Paulista, Dept Fis, Campina Grande, PB, Brazil
dc.description.affiliationUniv Fed Paraiba, Dept Fis, BR-58059970 Joao Pessoa, Paraiba, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, Dept Fis, Campina Grande, PB, Brazil
dc.format.extent77-83
dc.identifierhttp://dx.doi.org/10.1016/S0920-5632(03)02403-4
dc.identifier.citationNuclear Physics B-proceedings Supplements. Amsterdam: Elsevier Science Bv, v. 127, p. 77-83, 2004.
dc.identifier.doi10.1016/j.nuclphysbps.2003.12.012
dc.identifier.issn0920-5632
dc.identifier.urihttp://hdl.handle.net/11449/116680
dc.identifier.wosWOS:000189279000012
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofNuclear Physics B-proceedings Supplements
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.titleVacuum polarization by a magnetic flux in a cosmic string background.en
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.

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