Exotic massive 3D gravity
dc.contributor.author | Ozkan, M | |
dc.contributor.author | Pang, Y | |
dc.contributor.author | Townsend, PK | |
dc.date.accessioned | 2018-11-17T00:32:00Z | |
dc.date.available | 2018-11-17T00:32:00Z | |
dc.date.issued | 2018-08-09 | |
dc.identifier.issn | 1126-6708 | |
dc.identifier.uri | https://www.repository.cam.ac.uk/handle/1810/285389 | |
dc.description.abstract | The 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.language | eng | |
dc.publisher | Springer | |
dc.rights | Attribution 4.0 International | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.title | Exotic massive 3D gravity | |
dc.type | Article | |
prism.issueIdentifier | 8 | |
prism.publicationDate | 2018 | |
prism.publicationName | Journal of High Energy Physics | |
prism.volume | 2018 | |
dc.identifier.doi | 10.17863/CAM.32755 | |
dcterms.dateAccepted | 2018-08-03 | |
rioxxterms.versionofrecord | 10.1007/JHEP08(2018)035 | |
rioxxterms.licenseref.uri | http://creativecommons.org/licenses/by/4.0/ | |
rioxxterms.licenseref.startdate | 2018-08-09 | |
dc.contributor.orcid | Townsend, Paul [0000-0003-0311-9448] | |
dc.identifier.eissn | 1029-8479 | |
rioxxterms.type | Journal Article/Review | |
cam.issuedOnline | 2018-08-09 |
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