# Theory for multiple partially massless spin-2 fields

@article{Boulanger2019TheoryFM, title={Theory for multiple partially massless spin-2 fields}, author={N. Boulanger and C. Deffayet and S. Garcia-Saenz and L. Traina}, journal={Physical Review D}, year={2019} }

We revisit the problem of building consistent interactions for a multiplet of partially massless spin-2 fields in (anti-)de Sitter space. After rederiving and strengthening the existing no-go result on the impossibility of Yang-Mills type non-abelian deformations of the partially massless gauge algebra, we prove the uniqueness of the cubic interaction vertex and field-dependent gauge transformation that generalize the structures known from single-field analyses. Unlike in the case of one… Expand

#### 5 Citations

Interactions for Partially-Massless Spin-2 Fields

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Partially massless (PM) fields of spin-2 have been subject to renewed attention in recent years after the important advances made in the understanding of massive gravity [1,2]. In four-dimensional de… Expand

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A bstractWe find and classify the N=1$$ \mathcal{N}=1 $$ SUSY multiplets on AdS4 which contain partially massless fields. We do this by studying the non-unitary representations of the d = 3… Expand

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General Relativity can be reformulated as a diffeomorphism invariant gauge theory of the Lorentz group, with Lagrangian of the type f(F ∧ F ), where F is the curvature 2-form of the spin connection.… Expand

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We find and classify the simplest ${\cal N}=2$ SUSY multiplets on AdS$_4$ which contain partially massless fields. We do this by studying representations of the ${\cal N}=2$, $d=3$ superconformal… Expand

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We revisit the problem of building consistent interactions for a multiplet of partially massless spin-2 fields in (anti-)de Sitter space. After rederiving and strengthening the existing no-go result… Expand

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A bstractWe find and classify the N=1$$ \mathcal{N}=1 $$ SUSY multiplets on AdS4 which contain partially massless fields. We do this by studying the non-unitary representations of the d = 3… Expand