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dc.contributor.authorKAO, WFen_US
dc.date.accessioned2019-04-03T06:37:23Z-
dc.date.available2019-04-03T06:37:23Z-
dc.date.issued1993-04-15en_US
dc.identifier.issn0556-2821en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.47.3639en_US
dc.identifier.urihttp://hdl.handle.net/11536/3045-
dc.description.abstractWe study possible implications of a ten-dimensional Einstein-Kalb-Ramond theory. It is speculated that the compactification process and inflationary process axe closely related. It is also found that the torsion field tends to vanish after the inflation era is completed. This is in fact a general feature for the torsion Lagrangian. Hence the contribution from the Kalb-Ramond action is negligible effectively after the inflationary era. Some solutions to the field equations are also presented.en_US
dc.language.isoen_USen_US
dc.titleTORSION, COMPACTIFICATION, AND INFLATIONen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.47.3639en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume47en_US
dc.citation.issue8en_US
dc.citation.spage3639en_US
dc.citation.epage3642en_US
dc.contributor.department電子物理學系zh_TW
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.identifier.wosnumberWOS:A1993KY67400061en_US
dc.citation.woscount17en_US
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