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Covariant non-commutative space-time

Author(s): Heckman, Jonathan J.; Verlinde, Herman L.

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dc.contributor.authorHeckman, Jonathan J.-
dc.contributor.authorVerlinde, Herman L.-
dc.date.accessioned2019-04-04T17:23:30Z-
dc.date.available2019-04-04T17:23:30Z-
dc.date.issued2015-05en_US
dc.identifier.citationHeckman, Jonathan J, Verlinde, Herman. (2015). Covariant non-commutative space-time. NUCLEAR PHYSICS B, 894 (58 - 74). doi:10.1016/j.nuclphysb.2015.02.018en_US
dc.identifier.issn0550-3213-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr19q5v-
dc.description.abstractWe introduce a covariant non-commutative deformation of 3 + 1-dimensional conformal field theory. The deformation introduces a short-distance scale l(p), and thus breaks scale invariance, but preserves all space time isometries. The non-commutative algebra is defined on space times with non-zero constant curvature, i.e. dS(4) or AdS(4). The construction makes essential use of the representation of CFT tensor operators as polynomials in an auxiliary polarization tensor. The polarization tensor takes active part in the non-commutative algebra, which for dS(4) takes the form of so(5, 1), while for AdS(4) it assembles into so (4, 2). The structure of the non-commutative correlation functions hints that the deformed theory contains gravitational interactions and a Regge-like trajectory of higher spin excitations. (C) 2015 The Authors.en_US
dc.format.extent58 - 74en_US
dc.language.isoen_USen_US
dc.relation.ispartofNUCLEAR PHYSICS Ben_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleCovariant non-commutative space-timeen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1016/j.nuclphysb.2015.02.018-
dc.date.eissued2015-02-19en_US
dc.identifier.eissn1873-1562-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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