完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | Kao, WF | en_US |
dc.contributor.author | Lin, SY | en_US |
dc.contributor.author | Chyi, TK | en_US |
dc.date.accessioned | 2019-04-03T06:39:00Z | - |
dc.date.available | 2019-04-03T06:39:00Z | - |
dc.date.issued | 1996-02-15 | en_US |
dc.identifier.issn | 0556-2821 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.53.1955 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/1448 | - |
dc.description.abstract | The 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.iso | en_US | en_US |
dc.title | Weyl invariant black hole | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1103/PhysRevD.53.1955 | en_US |
dc.identifier.journal | PHYSICAL REVIEW D | en_US |
dc.citation.volume | 53 | en_US |
dc.citation.issue | 4 | en_US |
dc.citation.spage | 1955 | en_US |
dc.citation.epage | 1962 | en_US |
dc.contributor.department | 電子物理學系 | zh_TW |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Department of Electrophysics | en_US |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:A1996TW98200025 | en_US |
dc.citation.woscount | 8 | en_US |
顯示於類別: | 期刊論文 |