Abstract

We present higher-spin algebras containing a Poincaré subalgebra and with the same set of generators as the Lie algebras that are relevant to Vasiliev’s equations in any space-time dimension D ≥ 3. Given these properties, they can be considered either as candidate rigid symmetries for higher-spin gauge theories in Minkowski space or as Carrollian conformal higher-spin symmetries in one less dimension. We build these Lie algebras as quotients of the universal enveloping algebra of mathfrak{iso}left(1,D-1right) and we show how to recover them as Inönü-Wigner contractions of the rigid symmetries of higher-spin gauge theories in Anti de Sitter space or, equivalently, of relativistic conformal higher-spin symmetries. We use the same techniques to also define higher-spin algebras with the same set of generators and containing a Galilean conformal subalgebra, to be interpreted as non-relativistic limits of the conformal symmetries of a free scalar field. We begin by showing that the known flat-space higher-spin algebras in three dimensions can be obtained as quotients of the universal enveloping algebra of mathfrak{iso}left(1,2right) and then we extend the analysis along the same lines to a generic number of space-time dimensions. We also discuss the peculiarities that emerge for D = 5.

Highlights

  • The Poincaré and (Anti) de Sitter algebras describe the isometries of the vacuum in gravitational theories

  • They can be considered either as candidate rigid symmetries for higher-spin gauge theories in Minkowski space or as Carrollian conformal higher-spin symmetries in one less dimension. We build these Lie algebras as quotients of the universal enveloping algebra of iso(1, D − 1) and we show how to recover them as Inönü-Wigner contractions of the rigid symmetries of higher-spin gauge theories in Anti de Sitter space or, equivalently, of relativistic conformal higherspin symmetries

  • We focus on the global symmetries of gauge theories involving only Fronsdal’s fields in AdSD and on their construction as quotients of the universal enveloping algebra (UEA) of so(2, D − 1)

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Summary

Introduction

The Poincaré and (Anti) de Sitter algebras describe the isometries of the vacuum in gravitational theories. The situation is instead radically different in three-dimensional Minkowski space, where global higher-spin symmetries can be naturally obtained as Inönü-Wigner contractions of the AdS ones [16, 48–51] In this context, one can build interacting gauge theories using Chern-Simons actions as in AdS3, while specific interactions with matter were introduced following Vasiliev’s approach [52]. We start filling the gap by presenting bosonic higher-spin extensions of the Poincaré algebra in any space-time dimensions We reach this goal by classifying the quotients of the universal enveloping algebra of iso(1, D − 1) that have the same set of generators as the Lie algebras entering Vasiliev’s equations.

AdSD higher-spin algebras
Higher-spin “isometries” of the vacuum
Global symmetries for massless fields
Spacetime of generic dimension: the hsD algebra
Three dimensions: the hs3[λ] family
Five dimensions: the hs5[λ] family
Global symmetries for partially-massless fields: the AD[μ] family
Three space-time dimensions
Carrollian and Galilean contractions
The contracted algebras as quotients of U (iso(1, 2))
From U (so(2, 2)) to U (iso(1, 2))
Another Carrollian contraction
Alternative Ansatz for higher translations
Geometric realisation
Generic bulk dimension D ≥ 4
Minkowski/Carrollian-conformal basis for the hsD algebra
Higher-spin algebras from quotients of U (iso(1, D − 1))
Inönü-Wigner contractions of hsD
The particular case D = 5
Coset construction
Galilean-conformal higher-spin algebras in any dimensions
Galilean-conformal basis for the hsD algebra
Higher-spin algebras from quotients of U (gcaD−1)
Inönü-Wigner contractions reproducing the coset algebras
Alternative contractions and finite-dimensional algebras
Conclusions and outlook
Finite-dimensional matrix representations of hs5 M2 + 1
Full Text
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