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dc.contributor.authorKao, WFen_US
dc.contributor.authorLin, SYen_US
dc.contributor.authorChyi, TKen_US
dc.date.accessioned2019-04-03T06:39:00Z-
dc.date.available2019-04-03T06:39:00Z-
dc.date.issued1996-02-15en_US
dc.identifier.issn0556-2821en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.53.1955en_US
dc.identifier.urihttp://hdl.handle.net/11536/1448-
dc.description.abstractThe properties of the Weyl invariant black hole and its implications are studied. The calculation shows that there is no hair, up to a gauge choice, for a Weyl gauge field outside the event horizon of a black hole in the Weyl invariant limit. We also show that a scalar held will remain constant once the scale symmetry is broken spontaneously by the well-known Higgs potential. As a result, classical hair for the Weyl vector meson and scalar measuring field vanishes strictly in the presence of a spontaneously symmetry-breaking potential. Hence the no-hair theorem holds both in the Weyl invariant limit and the symmetry-breaking phase.en_US
dc.language.isoen_USen_US
dc.titleWeyl invariant black holeen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.53.1955en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume53en_US
dc.citation.issue4en_US
dc.citation.spage1955en_US
dc.citation.epage1962en_US
dc.contributor.department電子物理學系zh_TW
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:A1996TW98200025en_US
dc.citation.woscount8en_US
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