Anisotropic power-law inflation for the Dirac-Born-Infeld theory

Full metadata record

DC Field	Value	Language
dc.contributor.author	Do, Tuan Q.	en_US
dc.contributor.author	Kao, W. F.	en_US
dc.date.accessioned	2019-04-03T06:36:26Z	-
dc.date.available	2019-04-03T06:36:26Z	-
dc.date.issued	2011-12-28	en_US
dc.identifier.issn	2470-0010	en_US
dc.identifier.uri	http://dx.doi.org/10.1103/PhysRevD.84.123009	en_US
dc.identifier.uri	http://hdl.handle.net/11536/15029	-
dc.description.abstract	We find a new set of the Bianchi type I power-law expanding solutions in a string-motivated Dirac-Born-Infeld theory. Stability analysis shows that these power-law inflationary solutions remain stable with or without the contribution of the Dirac-Born-Infeld effect. We also find a new set of Bianchi type I expanding power-law solutions in a two scalar Dirac-Born-Infeld model with an additional phantom field. It is shown that the inclusion of the phantom field turns the Bianchi type I power-law solutions unstable during the inflationary phase.	en_US
dc.language.iso	en_US	en_US
dc.title	Anisotropic power-law inflation for the Dirac-Born-Infeld theory	en_US
dc.type	Article	en_US
dc.identifier.doi	10.1103/PhysRevD.84.123009	en_US
dc.identifier.journal	PHYSICAL REVIEW D	en_US
dc.citation.volume	84	en_US
dc.citation.issue	12	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:000298655600004	en_US
dc.citation.woscount	32	en_US
Appears in Collections:	Articles

Files in This Item:

If it is a zip file, please download the file and unzip it, then open index.html in a browser to view the full text content.