完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | Kao, W. F. | en_US |
dc.date.accessioned | 2014-12-08T15:07:32Z | - |
dc.date.available | 2014-12-08T15:07:32Z | - |
dc.date.issued | 2010-02-01 | en_US |
dc.identifier.issn | 1434-6044 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1140/epjc/s10052-009-1176-y | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/5928 | - |
dc.description.abstract | Inflationary higher derivative scalar-tensor theory is analyzed in this paper in a de Sitter background space. A useful model-independent formula of the Friedmann equation is derived and used to study the stability problem associated with the anisotropic perturbations of the inflationary solution. The stability conditions of the de Sitter solution are derived for a general class of models. For a simple demonstration, an induced gravity model is considered in this paper for the effects of the higher derivative interactions including a cubic term. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Scalar-tensor theory and the anisotropic perturbations of the inflationary universe | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1140/epjc/s10052-009-1176-y | en_US |
dc.identifier.journal | EUROPEAN PHYSICAL JOURNAL C | en_US |
dc.citation.volume | 65 | en_US |
dc.citation.issue | 3-4 | en_US |
dc.citation.spage | 555 | en_US |
dc.citation.epage | 565 | en_US |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:000274327200019 | - |
dc.citation.woscount | 1 | - |
顯示於類別: | 期刊論文 |