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 | 2019-04-03T06:42:30Z | - |
dc.date.available | 2019-04-03T06:42:30Z | - |
dc.date.issued | 2009-02-01 | en_US |
dc.identifier.issn | 1550-7998 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.79.043001 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/7655 | - |
dc.description.abstract | We show that a Brans-Dicke model admits some anisotropically inflating solutions which are identical to the solutions found in a higher derivative pure gravity theory. These inflating solutions were shown to break the cosmic no-hair theorem such that they do not approach the de Sitter universe at large times. The stability conditions of these solutions in this scalar-tensor theory are shown explicitly in this paper. It is shown that there exist unstable modes of the anisotropic perturbations. Therefore the inflating solutions are unstable in the scalar-tensor theory. | en_US |
dc.language.iso | en_US | en_US |
dc.title | Anisotropically inflating universes in a scalar-tensor theory | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1103/PhysRevD.79.043001 | en_US |
dc.identifier.journal | PHYSICAL REVIEW D | en_US |
dc.citation.volume | 79 | en_US |
dc.citation.issue | 4 | 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:000263816800007 | en_US |
dc.citation.woscount | 9 | en_US |
Appears in Collections: | Articles |
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