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Bianchi type I expanding universe in Weyl-invariant massive gravity

dc.citation.epage0en_US
dc.citation.issue6en_US
dc.citation.spage0en_US
dc.citation.volume90en_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.accessioned2019-04-03T06:37:51Z
dc.date.available2019-04-03T06:37:51Z
dc.date.issued2014-09-10en_US
dc.description.abstractWe will study the cosmological evolutions of aWeyl-invariant de Rham, Gabadadze, and Tolley (dRGT) massive gravity theory with a general fiducial metric. In the unitary gauge, this model is equivalent to a massive gauge field coupled to the dRGT massive gravity model. The massive gravity terms will serve as an effective cosmological constant for all metric spaces if the fiducial metric is treated as an auxiliary field. A further discussion will also be addressed on the bimetric theory. In particular, we will discuss the role played by the Weyl vector boson in Bianchi type I expanding space.en_US
dc.identifier.doi10.1103/PhysRevD.90.063003en_US
dc.identifier.issn2470-0010en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.90.063003en_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/124746
dc.identifier.wosnumberWOS:000353115700002en_US
dc.language.isoen_USen_US
dc.titleBianchi type I expanding universe in Weyl-invariant massive gravityen_US
dc.typeArticleen_US

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