DSpace at EWHA: The gravitational wave of the scalar-tensor theory

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DC Field	Value	Language
dc.contributor.author	김성원	*
dc.date.accessioned	2018-06-02T08:15:01Z	-
dc.date.available	2018-06-02T08:15:01Z	-
dc.date.issued	1998	*
dc.identifier.issn	0374-4884	*
dc.identifier.other	OAK-17095	*
dc.identifier.uri	https://dspace.ewha.ac.kr/handle/2015.oak/244362	-
dc.description.abstract	The gravitational wave is discussed in the general space-time with torsion and scalar field. It is shown that there are three types of wave equation: spin-0, spin-1, and spin-2 wave equations. When the effective stress-energy tensors for this gravitational wave is ejaculated, it is found that the additional term due to the scalar field affects them. The existence of the gravitational dipole moment by the spin is tested in the spin-1 vector wave equation.	*
dc.language	English	*
dc.title	The gravitational wave of the scalar-tensor theory	*
dc.type	Article	*
dc.relation.issue	SUPPL. 3	*
dc.relation.volume	33	*
dc.relation.index	SCI	*
dc.relation.index	SCIE	*
dc.relation.index	SCOPUS	*
dc.relation.index	KCI	*
dc.relation.startpage	S560	*
dc.relation.lastpage	S564	*
dc.relation.journaltitle	Journal of the Korean Physical Society	*
dc.identifier.scopusid	2-s2.0-0032278689	*
dc.author.google	Kim S.-W.	*
dc.contributor.scopusid	김성원(55862533800;57194851458)	*
dc.date.modifydate	20240116125219	*