Three-dimensional Spin-3 Theories Based on General Kinematical Algebras
Eric Bergshoeff, Daniel Grumiller, Stefan Prohazka, Jan Rosseel
TL;DR
This work extends Bacry–Lévy–Leblond’s kinematical classification to three-dimensional theories with massless spin-3 fields by classifying all IW contractions of the spin-3 $(A)dS_3$ algebras. It constructs corresponding Chern–Simons actions for ultra-relativistic Carroll and suitably extended non-relativistic (Extended Bargmann) algebras, providing linearized analyses and explicit invariant metrics. A key result is the Carroll case’s infinite-dimensional asymptotic symmetry via Carroll boundary conditions, suggesting similar extensions for the non-/ultra-relativistic spin-3 theories. The paper also develops spin-3 extensions of Extended Bargmann gravity through Medina–Revoy double extensions, enabling nondegenerate invariant bilinear forms and CS actions, thereby enriching the landscape of three-dimensional higher-spin gravity in non-AdS settings and offering avenues for holography, Hořava–Lifshitz connections, and condensed-matter applications.
Abstract
We initiate the study of non- and ultra-relativistic higher spin theories. For sake of simplicity we focus on the spin-3 case in three dimensions. We classify all kinematical algebras that can be obtained by all possible Inönü--Wigner contraction procedures of the kinematical algebra of spin-3 theory in three dimensional (anti-) de Sitter space-time. We demonstrate how to construct associated actions of Chern--Simons type, directly in the ultra-relativistic case and by suitable algebraic extensions in the non-relativistic case. We show how to give these kinematical algebras an infinite-dimensional lift by imposing suitable boundary conditions in a theory we call "Carroll Gravity", whose asymptotic symmetry algebra turns out to be an infinite-dimensional extension of the Carroll algebra.
