Kaluza-Klein induced gravity inflation
| dc.citation.epage | 0 | en_US |
| dc.citation.issue | 8 | en_US |
| dc.citation.spage | 0 | en_US |
| dc.citation.volume | 62 | 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 | 2000-10-15 | en_US |
| dc.description.abstract | A D-dimensional induced gravity theory is studied carefully in a 4 + (D-4) dimensional Friedmann-Robertson-Walker space-time. We try to extract information about the symmetry-breaking potential in search of an inflationary solution with a nonexpanding internal space. We find that the induced gravity model imposes strong constraints on the form of the symmetry-breaking potential in order to generate an acceptable inflationary universe. These constraints are analyzed carefully in this paper. | en_US |
| dc.identifier.doi | 10.1103/PhysRevD.62.084009 | 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.62.084009 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/30204 | |
| dc.identifier.wosnumber | WOS:000089977200034 | en_US |
| dc.language.iso | en_US | en_US |
| dc.title | Kaluza-Klein induced gravity inflation | en_US |
| dc.type | Article | en_US |