Higher-spin gravity as a theory on a fixed (anti) de Sitter background

10Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

We study Vasiliev’s higher-spin gravity in 3+1d. We formulate the theory in the so-called compensator formalism, where the local isometry group SO(4, 1) is reduced to the Lorentz group SO(3, 1) by a choice of spacelike direction in an internal 4+1d space. We present a consistent extension of Vasiliev’s equations that allows this internal direction to become spacetime-dependent. This allows a new point of view on the theory, where spacetime is identified with the de Sitter space of possible internal directions. We thus obtain an interacting theory of higher-spin massless gauge fields on a fixed, maximally symmetric background spacetime. We expect implications for the physical interpretation of higher-spin gravity, for the search for a Lagrangian formulation and/or quantization, as well as for higher-spin holography.

Cite

CITATION STYLE

APA

Neiman, Y. (2015). Higher-spin gravity as a theory on a fixed (anti) de Sitter background. Journal of High Energy Physics, 2015(4). https://doi.org/10.1007/JHEP04(2015)144

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free