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dc.contributor.author김성구-
dc.date.accessioned2016-08-28T11:08:43Z-
dc.date.available2016-08-28T11:08:43Z-
dc.date.issued1987-
dc.identifier.issn0556-2821-
dc.identifier.otherOAK-12653-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/228740-
dc.description.abstractVacuum polarization and spontaneous symmetry breaking in a two-dimensional massless fermion field theory with quartic interactions (the Gross-Neveu model) are studied in a cylindrical (R1×S1) space-time topology. In the case of untwisted fermion fields the symmetry-breaking behavior is similar to the model in Minkowski space-time except that the location of the effective potential minima depends upon the size of the space. In the case of a twisted fermion field there exists a critical size of the space such that the symmetry breaking occurs only for space larger than the critical one. © 1987 The American Physical Society.-
dc.languageEnglish-
dc.titleDynamical symmetry breaking and space-time topology-
dc.typeArticle-
dc.relation.issue10-
dc.relation.volume36-
dc.relation.indexSCOPUS-
dc.relation.startpage3172-
dc.relation.lastpage3177-
dc.relation.journaltitlePhysical Review D-
dc.identifier.doi10.1103/PhysRevD.36.3172-
dc.identifier.scopusid2-s2.0-0040446041-
dc.author.googleKim S.K.-
dc.author.googleNamgung W.-
dc.author.googleSoh K.S.-
dc.author.googleYee J.H.-
dc.contributor.scopusid김성구(22967145800)-
dc.date.modifydate20180104081001-


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