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Anisotropically inflating universes in a scalar-tensor theory

dc.citation.epage0en_US
dc.citation.issue4en_US
dc.citation.spage0en_US
dc.citation.volume79en_US
dc.citation.woscount9en_US
dc.contributor.authorKao, W. F.en_US
dc.contributor.authorLin, Ing-Chenen_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.date.accessioned2019-04-03T06:42:30Z
dc.date.available2019-04-03T06:42:30Z
dc.date.issued2009-02-01en_US
dc.description.abstractWe 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.identifier.doi10.1103/PhysRevD.79.043001en_US
dc.identifier.issn1550-7998en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.79.043001en_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/7655
dc.identifier.wosnumberWOS:000263816800007en_US
dc.language.isoen_USen_US
dc.titleAnisotropically inflating universes in a scalar-tensor theoryen_US
dc.typeArticleen_US

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