Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kao, WF | en_US |
dc.date.accessioned | 2019-04-03T06:39:33Z | - |
dc.date.available | 2019-04-03T06:39:33Z | - |
dc.date.issued | 2000-02-15 | en_US |
dc.identifier.issn | 2470-0010 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.61.044004 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/30727 | - |
dc.description.abstract | We 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.iso | en_US | en_US |
dc.title | Magnetic monopole in induced Einstein-Yang-Mills models | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1103/PhysRevD.61.044004 | en_US |
dc.identifier.journal | PHYSICAL REVIEW D | en_US |
dc.citation.volume | 61 | en_US |
dc.citation.issue | 4 | en_US |
dc.citation.spage | 0 | en_US |
dc.citation.epage | 0 | en_US |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:000085383200020 | en_US |
dc.citation.woscount | 2 | en_US |
Appears in Collections: | Articles |
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