Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kao, W. F. | en_US |
dc.contributor.author | Lin, Ing-Chen | en_US |
dc.date.accessioned | 2014-12-08T15:10:23Z | - |
dc.date.available | 2014-12-08T15:10:23Z | - |
dc.date.issued | 2009-01-01 | en_US |
dc.identifier.issn | 1475-7516 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1088/1475-7516/2009/01/022 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/7936 | - |
dc.description.abstract | Stability 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.iso | en_US | en_US |
dc.subject | cosmological perturbation theory | en_US |
dc.subject | physics of the early universe | en_US |
dc.title | Stability conditions for the Bianchi type II anisotropically inflating universes | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1088/1475-7516/2009/01/022 | en_US |
dc.identifier.journal | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | en_US |
dc.citation.volume | en_US | |
dc.citation.issue | 1 | en_US |
dc.citation.epage | en_US | |
dc.contributor.department | 物理研究所 | zh_TW |
dc.contributor.department | Institute of Physics | en_US |
dc.identifier.wosnumber | WOS:000263824000022 | - |
dc.citation.woscount | 5 | - |
Appears in Collections: | Articles |
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