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SCALE-INVARIANT EFFECTIVE ACTION WITH TORSION

dc.citation.epage241en_US
dc.citation.issue4en_US
dc.citation.spage238en_US
dc.citation.volume70en_US
dc.citation.woscount1
dc.contributor.authorKAO, WFen_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.departmentNational Chiao Tung Universityen_US
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.date.accessioned2014-12-08T15:04:56Z
dc.date.available2014-12-08T15:04:56Z
dc.date.issued1992-04-01en_US
dc.description.abstractWe 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.issn0008-4204en_US
dc.identifier.journalCANADIAN JOURNAL OF PHYSICSen_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/3459
dc.identifier.wosnumberWOS:A1992JC71000007
dc.language.isoen_USen_US
dc.titleSCALE-INVARIANT EFFECTIVE ACTION WITH TORSIONen_US
dc.typeArticleen_US

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