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dc.contributor.authorDo, Tuan Q.en_US
dc.contributor.authorKao, W. F.en_US
dc.date.accessioned2019-04-03T06:43:37Z-
dc.date.available2019-04-03T06:43:37Z-
dc.date.issued2013-09-05en_US
dc.identifier.issn2470-0010en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.88.063006en_US
dc.identifier.urihttp://hdl.handle.net/11536/22760-
dc.description.abstractWe study the cosmological implications of a ghost-free nonlinear massive gravity theory with a cosmological constant. We find that the massive terms serve as an effective cosmological constant for a large class of metric spaces with a compatible fiducial metric associated with the massive terms. A specific solution is solved as an example for this model under the Bianchi type I space and a compatible Bianchi type I fiducial metric. A stability analysis indicates that this set of solutions tends to be stable. Nonetheless, the anisotropically expanding solution will, in general, turn unstable when an additional scalar field with negative kinetic energy is introduced.en_US
dc.language.isoen_USen_US
dc.titleAnisotropically expanding universe in massive gravityen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.88.063006en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume88en_US
dc.citation.issue6en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000324053700004en_US
dc.citation.woscount14en_US
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