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

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniv Fed Paraiba
dc.date.accessioned2015-03-18T15:53:43Z
dc.date.available2015-03-18T15:53:43Z
dc.date.created2015-03-18T15:53:43Z
dc.date.issued2004-02-01
dc.identifierNuclear Physics B-proceedings Supplements. Amsterdam: Elsevier Science Bv, v. 127, p. 77-83, 2004.
dc.identifier0920-5632
dc.identifierhttp://hdl.handle.net/11449/116680
dc.identifier10.1016/j.nuclphysbps.2003.12.012
dc.identifierWOS:000189279000012
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.
dc.languageeng
dc.publisherElsevier B.V.
dc.relationNuclear Physics B-proceedings Supplements
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.titleVacuum polarization by a magnetic flux in a cosmic string background.
dc.typeArtículos de revistas


Este ítem pertenece a la siguiente institución