Scalar-tensor theory and the anisotropic perturbations of the inflationary universe

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DC Field	Value	Language
dc.contributor.author	Kao, W. F.	en_US
dc.date.accessioned	2014-12-08T15:07:32Z	-
dc.date.available	2014-12-08T15:07:32Z	-
dc.date.issued	2010-02-01	en_US
dc.identifier.issn	1434-6044	en_US
dc.identifier.uri	http://dx.doi.org/10.1140/epjc/s10052-009-1176-y	en_US
dc.identifier.uri	http://hdl.handle.net/11536/5928	-
dc.description.abstract	Inflationary higher derivative scalar-tensor theory is analyzed in this paper in a de Sitter background space. A useful model-independent formula of the Friedmann equation is derived and used to study the stability problem associated with the anisotropic perturbations of the inflationary solution. The stability conditions of the de Sitter solution are derived for a general class of models. For a simple demonstration, an induced gravity model is considered in this paper for the effects of the higher derivative interactions including a cubic term.	en_US
dc.language.iso	en_US	en_US
dc.title	Scalar-tensor theory and the anisotropic perturbations of the inflationary universe	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1140/epjc/s10052-009-1176-y	en_US
dc.identifier.journal	EUROPEAN PHYSICAL JOURNAL C	en_US
dc.citation.volume	65	en_US
dc.citation.issue	3-4	en_US
dc.citation.spage	555	en_US
dc.citation.epage	565	en_US
dc.contributor.department	物理研究所	zh_TW
dc.contributor.department	Institute of Physics	en_US
dc.identifier.wosnumber	WOS:000274327200019	-
dc.citation.woscount	1	-
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