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dc.contributor.authorKao, WFen_US
dc.date.accessioned2019-04-03T06:39:33Z-
dc.date.available2019-04-03T06:39:33Z-
dc.date.issued2000-02-15en_US
dc.identifier.issn2470-0010en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.61.044004en_US
dc.identifier.urihttp://hdl.handle.net/11536/30727-
dc.description.abstractWe show that a regular SO(3) non-Abelian monopole cannot exist in induced gravity models with a variety of symmetry breaking potentials. The no-hair theorem is also shown to be true in these models. We also analyze the global behavior of the gauge field in the presence of a black hole with a nonvanishing cosmological constant. It is shown that the nontrivial non-Abelian monopole solution exists only if the radius of the event horizon is smaller than the characteristic radius of the classical monopole.en_US
dc.language.isoen_USen_US
dc.titleMagnetic monopole in induced Einstein-Yang-Mills modelsen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.61.044004en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume61en_US
dc.citation.issue4en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000085383200020en_US
dc.citation.woscount2en_US
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