Kaluza-Klein induced gravity inflation

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DC Field	Value	Language
dc.contributor.author	Kao, WF	en_US
dc.date.accessioned	2019-04-03T06:39:29Z	-
dc.date.available	2019-04-03T06:39:29Z	-
dc.date.issued	2000-10-15	en_US
dc.identifier.issn	2470-0010	en_US
dc.identifier.uri	http://dx.doi.org/10.1103/PhysRevD.62.084009	en_US
dc.identifier.uri	http://hdl.handle.net/11536/30204	-
dc.description.abstract	A D-dimensional induced gravity theory is studied carefully in a 4 + (D-4) dimensional Friedmann-Robertson-Walker space-time. We try to extract information about the symmetry-breaking potential in search of an inflationary solution with a nonexpanding internal space. We find that the induced gravity model imposes strong constraints on the form of the symmetry-breaking potential in order to generate an acceptable inflationary universe. These constraints are analyzed carefully in this paper.	en_US
dc.language.iso	en_US	en_US
dc.title	Kaluza-Klein induced gravity inflation	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1103/PhysRevD.62.084009	en_US
dc.identifier.journal	PHYSICAL REVIEW D	en_US
dc.citation.volume	62	en_US
dc.citation.issue	8	en_US
dc.citation.spage	0	en_US
dc.citation.epage	0	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000089977200034	en_US
dc.citation.woscount	5	en_US
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