SCALE-INVARIANT EFFECTIVE ACTION WITH TORSION
| dc.citation.epage | 241 | en_US |
| dc.citation.issue | 4 | en_US |
| dc.citation.spage | 238 | en_US |
| dc.citation.volume | 70 | 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 | 2014-12-08T15:04:56Z | |
| dc.date.available | 2014-12-08T15:04:56Z | |
| dc.date.issued | 1992-04-01 | en_US |
| dc.description.abstract | We considered a four-dimensional scale-invariant effective theory with a torsion field conformally coupled to a metric field. We find that the contribution from the torsion field is negligible in the evolution of the early universe. An exact solution is also obtained for k = 0 Friedmann-Robertson-Walker space in the vanishing cosmological constant limit. This solution is also a good approximation to k not-equal 0 spaces. Possible implications to the inflationary universe are also discussed. | en_US |
| dc.identifier.issn | 0008-4204 | en_US |
| dc.identifier.journal | CANADIAN JOURNAL OF PHYSICS | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/3459 | |
| dc.identifier.wosnumber | WOS:A1992JC71000007 | |
| dc.language.iso | en_US | en_US |
| dc.title | SCALE-INVARIANT EFFECTIVE ACTION WITH TORSION | en_US |
| dc.type | Article | en_US |
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