2017
DOI: 10.1140/epjc/s10052-017-5189-7
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Weyl and transverse diffeomorphism invariant spin-2 models in $$D=2+1$$ D = 2 + 1

Abstract: There are two covariant descriptions of massless spin-2 particles in D = 3 + 1 via a symmetric rank-2 tensor: the linearized Einstein-Hilbert (LEH) theory and the Weyl plus transverse diffeomorphism (WTDIFF) invariant model. From the LEH theory one can obtain the linearized new massive gravity (NMG) in D = 2 + 1 via Kaluza-Klein dimensional reduction followed by a dual master action. Here we show that a similar route takes us from the WTDIFF model to a linearized scalar-tensor NMG which belongs to a larger cla… Show more

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Cited by 3 publications
(8 citation statements)
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“…For instance, in the s = 2 case there are two choices for the D-tensor, one corresponds to the linearized Einstein-Hilbert theory and the other one to the WTDiff model or linearized unimodular gravity, both Lagrangians have no propagating modes in D = 2 + 1. The respective self-dual models L SD 2s−1 are the linearized topologically massive gravity [1] and linearized unimodular topologically massive gravity [23]. One can also combine L (s) 2s and L (s) 2s−2 and build up doublet models L D 2s containing both helicities +s and −s.…”
Section: General Set Upmentioning
confidence: 99%
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“…For instance, in the s = 2 case there are two choices for the D-tensor, one corresponds to the linearized Einstein-Hilbert theory and the other one to the WTDiff model or linearized unimodular gravity, both Lagrangians have no propagating modes in D = 2 + 1. The respective self-dual models L SD 2s−1 are the linearized topologically massive gravity [1] and linearized unimodular topologically massive gravity [23]. One can also combine L (s) 2s and L (s) 2s−2 and build up doublet models L D 2s containing both helicities +s and −s.…”
Section: General Set Upmentioning
confidence: 99%
“…One can also combine L (s) 2s and L (s) 2s−2 and build up doublet models L D 2s containing both helicities +s and −s. They represent higher spin analogues of the linearized NMG [17] and of the linearized unimodular NMG [23]. In the next section, as a preparation for the section 4 where possible choices for D µ 1 µ 2 •••µs will be discussed, we give closed formulae for the Cotton tensor and its symmetrized curl on the flat space.…”
Section: General Set Upmentioning
confidence: 99%
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