Bianchi type I anisotropic power-law solutions for the Galileon models
| dc.citation.epage | 0 | en_US |
| dc.citation.issue | 2 | en_US |
| dc.citation.spage | 0 | en_US |
| dc.citation.volume | 96 | en_US |
| dc.citation.woscount | 6 | en_US |
| dc.contributor.author | Do, Tuan Q. | en_US |
| dc.contributor.author | Kao, W. F. | en_US |
| dc.contributor.department | 物理研究所 | zh_TW |
| dc.contributor.department | Institute of Physics | en_US |
| dc.date.accessioned | 2019-04-03T06:43:20Z | |
| dc.date.available | 2019-04-03T06:43:20Z | |
| dc.date.issued | 2017-07-25 | en_US |
| dc.description.abstract | We will study the cosmological solutions of a class of Galileon models. A special class of the Bianchi type I power-law solutions will be presented in this paper. We will show that these Bianchi type I power-law solutions are stable during the inflationary phase. In addition, we will also show that the presence of a phantom field induces at least an unstable mode for the perturbation equation and destabilizes the power-law solutions. | en_US |
| dc.identifier.doi | 10.1103/PhysRevD.96.023529 | en_US |
| dc.identifier.issn | 2470-0010 | en_US |
| dc.identifier.journal | PHYSICAL REVIEW D | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.96.023529 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/145835 | |
| dc.identifier.wosnumber | WOS:000406308600005 | en_US |
| dc.language.iso | en_US | en_US |
| dc.title | Bianchi type I anisotropic power-law solutions for the Galileon models | en_US |
| dc.type | Article | en_US |