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dc.contributor.author최강신*
dc.date.accessioned2018-12-07T16:30:37Z-
dc.date.available2018-12-07T16:30:37Z-
dc.date.issued2017*
dc.identifier.issn0370-2693*
dc.identifier.otherOAK-20820*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/247372-
dc.description.abstractGauge symmetries are known to be respected by gravity because gauge charges carry flux lines, but global charges do not carry flux lines and are not conserved by gravitational interaction. For discrete symmetries, they are spontaneously broken in the Universe, forming domain walls. Since the realization of discrete symmetries in the Universe must involve the vacuum expectation values of Higgs fields, a string-like configuration (hair) at the intersection of domain walls in the Higgs vacua can be realized. Therefore, we argue that discrete charges are also respected by gravity. © 2017 The Author(s)*
dc.description.sponsorshipMinistry of Education, Science and Technology*
dc.languageEnglish*
dc.publisherElsevier B.V.*
dc.subjectDiscrete hair*
dc.subjectDiscrete symmetry*
dc.subjectGravity*
dc.subjectWormholes*
dc.titleHairs of discrete symmetries and gravity*
dc.typeArticle*
dc.relation.volume769*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.startpage430*
dc.relation.lastpage435*
dc.relation.journaltitlePhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics*
dc.identifier.doi10.1016/j.physletb.2017.04.008*
dc.identifier.wosidWOS:000402342500065*
dc.identifier.scopusid2-s2.0-85028516196*
dc.author.googleChoi K.S.*
dc.author.googleKim J.E.*
dc.author.googleKyae B.*
dc.author.googleNam S.*
dc.contributor.scopusid최강신(56289191500)*
dc.date.modifydate20240220111904*


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