SPATIAL DEPENDENCE OF INFLATON IN THE PRESENCE OF THE TORSION FIELD
| dc.citation.epage | 158 | en_US |
| dc.citation.issue | 3 | en_US |
| dc.citation.spage | 155 | en_US |
| dc.citation.volume | 163 | en_US |
| dc.citation.woscount | 1 | |
| dc.contributor.author | KAO, WF | en_US |
| dc.contributor.department | 交大名義發表 | zh_TW |
| dc.contributor.department | 電子物理學系 | zh_TW |
| dc.contributor.department | National Chiao Tung University | en_US |
| dc.contributor.department | Department of Electrophysics | en_US |
| dc.date.accessioned | 2014-12-08T15:04:57Z | |
| dc.date.available | 2014-12-08T15:04:57Z | |
| dc.date.issued | 1992-03-16 | en_US |
| dc.description.abstract | We show that, in a class of induced gravity models with (or without) torsion, the associated scalar field (the inflaton) has to be spatial independent in order to admit a Robertson-Walker type solution. Details of the proof are presented. The proof requires a great deal of mathematics which also serves as a pedagogical exercise by itself. | en_US |
| dc.identifier.issn | 0375-9601 | en_US |
| dc.identifier.journal | PHYSICS LETTERS A | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/3483 | |
| dc.identifier.wosnumber | WOS:A1992HM76900004 | |
| dc.language.iso | en_US | en_US |
| dc.title | SPATIAL DEPENDENCE OF INFLATON IN THE PRESENCE OF THE TORSION FIELD | en_US |
| dc.type | Article | en_US |
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