完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | Do, Tuan Q. | en_US |
dc.contributor.author | Kao, W. F. | en_US |
dc.contributor.author | Lin, Ing-Chen | en_US |
dc.date.accessioned | 2019-04-03T06:35:58Z | - |
dc.date.available | 2019-04-03T06:35:58Z | - |
dc.date.issued | 2011-06-07 | en_US |
dc.identifier.issn | 1550-7998 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.83.123002 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/22714 | - |
dc.description.abstract | A special class of Bianchi type I expanding solutions in a string motivated theory with a single scalar field has been speculated to break the cosmic no-hair theorem that will not approach the late time isotropic expanding solution. We will show by a new perturbation approach that an unstable mode for the inflationary solutions exists when an additional phantom field is introduced. The result indicates that the existence of an unstable mode is closely related to the extra fields that could be present during the very early Universe. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Anisotropic power-law inflation for a two scalar fields model | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1103/PhysRevD.83.123002 | en_US |
dc.identifier.journal | PHYSICAL REVIEW D | en_US |
dc.citation.volume | 83 | en_US |
dc.citation.issue | 12 | 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:000291353700001 | en_US |
dc.citation.woscount | 43 | en_US |
顯示於類別: | 期刊論文 |