Bianchi type-I space and the stability of the inflationary Friedmann-Robertson-Walker solution
| dc.citation.epage | 0 | en_US |
| dc.citation.issue | 10 | en_US |
| dc.citation.spage | 0 | en_US |
| dc.citation.volume | 64 | en_US |
| dc.citation.woscount | 5 | en_US |
| dc.contributor.author | Kao, WF | en_US |
| dc.contributor.department | 物理研究所 | zh_TW |
| dc.contributor.department | Institute of Physics | en_US |
| dc.date.accessioned | 2019-04-03T06:39:29Z | |
| dc.date.available | 2019-04-03T06:39:29Z | |
| dc.date.issued | 2001-11-15 | en_US |
| dc.description.abstract | A stability analysis of the Bianchi type-I universe in pure gravity theory is studied in detail, We first derive the nonredundant field equation of the system by introducing the generalized Bianchi type-I metric. This nonredundant equation reduces to the Friedmann equation in the isotropic limit. It is shown further that any unstable mode of the isotropic perturbation with respect to a de Sitter background is also unstable with respect to anisotropic perturbations. The implications of the choice of physical theories are discussed in detail in this paper. | en_US |
| dc.identifier.doi | 10.1103/PhysRevD.64.107301 | 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.64.107301 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/29252 | |
| dc.identifier.wosnumber | WOS:000172074100074 | en_US |
| dc.language.iso | en_US | en_US |
| dc.title | Bianchi type-I space and the stability of the inflationary Friedmann-Robertson-Walker solution | en_US |
| dc.type | Article | en_US |