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Magnetically charged black holes in induced gravity

dc.citation.epage704en_US
dc.citation.issue5en_US
dc.citation.spage693en_US
dc.citation.volume36en_US
dc.citation.woscount1
dc.contributor.authorDai, WBen_US
dc.contributor.authorKao, WFen_US
dc.contributor.authorWang, SYen_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.date.accessioned2014-12-08T15:47:30Z
dc.date.available2014-12-08T15:47:30Z
dc.date.issued1998-10-01en_US
dc.description.abstractIt is shown that the regular SO3 non-abelian spherically symmetric monopole solution does not exist in an induced Einstein-Yang-Mills-Higgs model. It is also shown that Higgs scalar hair cannot exist in the presence of a black hole event horizon in this model. The corresponding global behavior of the gauge field is analyzed in a black hole background. In particular, it is shown that a non-trivial 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.identifier.issn0577-9073en_US
dc.identifier.journalCHINESE JOURNAL OF PHYSICSen_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/31834
dc.identifier.wosnumberWOS:000076321600005
dc.language.isoen_USen_US
dc.titleMagnetically charged black holes in induced gravityen_US
dc.typeArticleen_US

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