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dc.contributor.authorKao, W. F.en_US
dc.contributor.authorLin, Ing-Chenen_US
dc.date.accessioned2014-12-08T15:10:23Z-
dc.date.available2014-12-08T15:10:23Z-
dc.date.issued2009-01-01en_US
dc.identifier.issn1475-7516en_US
dc.identifier.urihttp://dx.doi.org/10.1088/1475-7516/2009/01/022en_US
dc.identifier.urihttp://hdl.handle.net/11536/7936-
dc.description.abstractStability conditions for a class of anisotropically inflating solutions in the Bianchi type II background space are shown explicitly in this paper. These inflating solutions were known to break the cosmic no-hair theorem such that they do not approach the de Sitter universe at large times. It can be shown that unstable modes of the anisotropic perturbations always exist for this class of expanding solutions. As a result, we show that these set of anisotropically expanding solutions are unstable against anisotropic perturbations in the Bianchi type II space.en_US
dc.language.isoen_USen_US
dc.subjectcosmological perturbation theoryen_US
dc.subjectphysics of the early universeen_US
dc.titleStability conditions for the Bianchi type II anisotropically inflating universesen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/1475-7516/2009/01/022en_US
dc.identifier.journalJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICSen_US
dc.citation.volumeen_US
dc.citation.issue1en_US
dc.citation.epageen_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000263824000022-
dc.citation.woscount5-
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