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dc.contributor.author김성원*
dc.date.accessioned2018-06-02T08:15:15Z-
dc.date.available2018-06-02T08:15:15Z-
dc.date.issued1996*
dc.identifier.issn0374-4884*
dc.identifier.otherOAK-16974*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/244451-
dc.description.abstractIn this paper the Brans-Dicke cosmological model with torsion is considered. The effects of the spin and the scalar field on the expansion rate and the types of inflation are discussed. It is shown that the expansion rate is faster than the extended inflation.*
dc.languageEnglish*
dc.titleBrans-dicke cosmological model with torsion*
dc.typeArticle*
dc.relation.issueSUPPL. 4*
dc.relation.volume28*
dc.relation.indexSCI*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.indexKCI*
dc.relation.startpageS519*
dc.relation.lastpageS524*
dc.relation.journaltitleJournal of the Korean Physical Society*
dc.identifier.scopusid2-s2.0-0030516169*
dc.author.googleKim S.-W.*
dc.author.googleKim S.P.*
dc.author.googleLee J.*
dc.author.googlePark D.H.*
dc.contributor.scopusid김성원(55862533800;57194851458)*
dc.date.modifydate20240116125219*
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사범대학 > 과학교육과 > Journal papers
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