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Homogeneous anisotropic solutions of topologically massive gravity with a cosmological constant and their homogeneous deformations

dc.citation.epageen_US
dc.citation.issue12en_US
dc.citation.volume30en_US
dc.citation.woscount1
dc.contributor.authorMoutsopoulos, Georgeen_US
dc.contributor.department電子物理學系zh_TW
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.date.accessioned2014-12-08T15:31:22Z
dc.date.available2014-12-08T15:31:22Z
dc.date.issued2013-06-21en_US
dc.description.abstractWe solve the equations of topologically massive gravity (TMG) with a potentially non-vanishing cosmological constant for homogeneous metrics without isotropy. We only reproduce known solutions. We also discuss their homogeneous deformations, possibly with isotropy. We show that de Sitter space and hyperbolic space cannot be infinitesimally homogeneously deformed in TMG. We clarify some of their Segre-Petrov types and discuss the warped de Sitter spacetime.en_US
dc.identifier.doi10.1088/0264-9381/30/12/125014en_US
dc.identifier.issn0264-9381en_US
dc.identifier.journalCLASSICAL AND QUANTUM GRAVITYen_US
dc.identifier.urihttp://dx.doi.org/10.1088/0264-9381/30/12/125014en_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/22287
dc.identifier.wosnumberWOS:000319664000015
dc.language.isoen_USen_US
dc.titleHomogeneous anisotropic solutions of topologically massive gravity with a cosmological constant and their homogeneous deformationsen_US
dc.typeArticleen_US

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