Bianchi type I anisotropic power-law solutions for the Galileon models

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DC Field	Value	Language
dc.contributor.author	Do, Tuan Q.	en_US
dc.contributor.author	Kao, W. F.	en_US
dc.date.accessioned	2019-04-03T06:43:20Z	-
dc.date.available	2019-04-03T06:43:20Z	-
dc.date.issued	2017-07-25	en_US
dc.identifier.issn	2470-0010	en_US
dc.identifier.uri	http://dx.doi.org/10.1103/PhysRevD.96.023529	en_US
dc.identifier.uri	http://hdl.handle.net/11536/145835	-
dc.description.abstract	We will study the cosmological solutions of a class of Galileon models. A special class of the Bianchi type I power-law solutions will be presented in this paper. We will show that these Bianchi type I power-law solutions are stable during the inflationary phase. In addition, we will also show that the presence of a phantom field induces at least an unstable mode for the perturbation equation and destabilizes the power-law solutions.	en_US
dc.language.iso	en_US	en_US
dc.title	Bianchi type I anisotropic power-law solutions for the Galileon models	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1103/PhysRevD.96.023529	en_US
dc.identifier.journal	PHYSICAL REVIEW D	en_US
dc.citation.volume	96	en_US
dc.citation.issue	2	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:000406308600005	en_US
dc.citation.woscount	6	en_US
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