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dc.contributor.authorOzkan, M
dc.contributor.authorPang, Y
dc.contributor.authorTownsend, Paul
dc.date.accessioned2018-11-17T00:32:00Z
dc.date.available2018-11-17T00:32:00Z
dc.date.issued2018-08-09
dc.identifier.issn1126-6708
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/285389
dc.description.abstractThe linearized equations of “New Massive Gravity” propagate a parity doublet of massive spin-2 modes in 3D Minkowski spacetime, but a different non-linear extension is made possible by “third-way” consistency. There is a “Chern-Simons-like” action, as for other 3D massive gravity models, but the new theory is “exotic”: its action is parity odd. This “Exotic Massive Gravity” is the next-to-simplest case in an infinite sequence of third-way consistent 3D gravity theories, the simplest being the “Minimal Massive Gravity” alternative to “Topologically Massive Gravity”.
dc.languageeng
dc.publisherSpringer
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleExotic massive 3D gravity
dc.typeArticle
prism.issueIdentifier8
prism.publicationDate2018
prism.publicationNameJournal of High Energy Physics
prism.volume2018
dc.identifier.doi10.17863/CAM.32755
dcterms.dateAccepted2018-08-03
rioxxterms.versionofrecord10.1007/JHEP08(2018)035
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
rioxxterms.licenseref.startdate2018-08-09
dc.contributor.orcidTownsend, Paul [0000-0003-0311-9448]
dc.identifier.eissn1029-8479
dc.publisher.urlhttps://link.springer.com/article/10.1007/JHEP08(2018)035
rioxxterms.typeJournal Article/Review
cam.issuedOnline2018-08-09
dc.identifier.urlhttps://link.springer.com/article/10.1007/JHEP08(2018)035


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Attribution 4.0 International
Except where otherwise noted, this item's licence is described as Attribution 4.0 International