DSpace at EWHA: The cosmological model with scalar, spin and torsion field

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DC Field	Value	Language
dc.contributor.author	김성원	*
dc.date.accessioned	2018-06-02T08:14:47Z	-
dc.date.available	2018-06-02T08:14:47Z	-
dc.date.issued	1997	*
dc.identifier.issn	0369-3554	*
dc.identifier.other	OAK-17301	*
dc.identifier.uri	https://dspace.ewha.ac.kr/handle/2015.oak/244271	-
dc.description.abstract	In this paper the Brans-Dicke cosmological model with spin and torsion field is considered. The effects of the spin and the scalar field on the expansion rate and the types of inflation are discussed. Since the torsion field is generated by the scalar field as well as by the spin, the torsion effect by the scalar field still remains even if there are no spins. It is shown that the expansion rate is the power law faster than the extended inflation. The bubble nucleation rates are the same as in the usual Brans-Dicke case.	*
dc.language	English	*
dc.title	The cosmological model with scalar, spin and torsion field	*
dc.type	Article	*
dc.relation.issue	2-3	*
dc.relation.volume	112	*
dc.relation.index	SCOPUS	*
dc.relation.startpage	363	*
dc.relation.lastpage	373	*
dc.relation.journaltitle	Nuovo Cimento della Societa Italiana di Fisica B	*
dc.identifier.scopusid	2-s2.0-0040052645	*
dc.author.google	Kim S.-W.	*
dc.contributor.scopusid	김성원(55862533800;57194851458)	*
dc.date.modifydate	20240116125219	*