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.date.accessioned | 2018-08-21T05:53:39Z | - |
dc.date.available | 2018-08-21T05:53:39Z | - |
dc.date.issued | 2018-05-08 | en_US |
dc.identifier.issn | 1434-6044 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1140/epjc/s10052-018-5846-5 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/144983 | - |
dc.description.abstract | A set of power-law solutions of a conformal-violating Maxwell model with a non-standard scalar-vector coupling will be shown in this paper. In particular, we are interested in a coupling term of the form X(2n)F(mu v)F(mu v )with X denoting the kinetic term of the scalar field. Stability analysis indicates that the new set of anisotropic power-law solutions is unstable during the inflationary phase. The result is consistent with the cosmic no-hair conjecture. We show, however, that a set of stable slowly expanding solutions does exist for a small range of parameters lambda and n. Hence a small anisotropy can survive during the slowly expanding phase. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Anisotropic power-law inflation for a conformal-violating Maxwell model | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1140/epjc/s10052-018-5846-5 | en_US |
dc.identifier.journal | EUROPEAN PHYSICAL JOURNAL C | en_US |
dc.citation.volume | 78 | en_US |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:000432077200003 | en_US |
顯示於類別: | 期刊論文 |