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Black Holes and Singularity Resolution in Higher Spin Gravity

Alejandra Castro, Eliot Hijano, Arnaud Lepage-Jutier, Alexander Maloney

TL;DR

The paper investigates higher spin gravity in AdS$_3$ with gauge group SL(N,R)×SL(N,R), showing that higher spin gauge transformations modify geometric notions like curvature and causality, and can render apparent singularities gauge artifacts. Solutions are classified by holonomies around non-contractible cycles, with the N=3 case analyzed to reveal how different embeddings (principal vs diagonal) yield distinct gravitational interpretations while sharing holonomy data. The authors construct explicit SL(3,R) black hole solutions, derive their thermodynamics, and demonstrate singularity resolution via gauge transformations, linking the bulk holonomies to boundary CFT data through extended algebras. This work provides a concrete, tractable framework for black hole thermodynamics in theories with extended gauge symmetry and highlights the embedding-dependent relation between geometry and higher spin charges.

Abstract

We investigate higher spin theories of gravity in three dimensions based on the gauge group SL(N,R)*SL(N,R). In these theories the usual diffeomorphism symmetry is enhanced to include higher spin gauge transformations under which traditional geometric notions of curvature and causality are no longer invariant. This implies, for example, that apparently singular geometries can be rendered smooth by a gauge transformation, much like the resolution of orbifold singularities in string theory. The classical solutions, including the recently constructed higher spin black hole, are characterized by their holonomies around the non-contractible cycles of space-time. The black hole solutions are shown to be gauge equivalent to a BTZ black hole which is charged under a set of U(1) Chern-Simons fields. Nevertheless, depending on the choice of embedding of the gravitational gauge group, the space-time geometry may be non-trivial. We study in detail the N=3 example, where this observation allows us to find a gauge where the black hole geometry takes a simple form and the thermodynamic properties can be studied.

Black Holes and Singularity Resolution in Higher Spin Gravity

TL;DR

The paper investigates higher spin gravity in AdS with gauge group SL(N,R)×SL(N,R), showing that higher spin gauge transformations modify geometric notions like curvature and causality, and can render apparent singularities gauge artifacts. Solutions are classified by holonomies around non-contractible cycles, with the N=3 case analyzed to reveal how different embeddings (principal vs diagonal) yield distinct gravitational interpretations while sharing holonomy data. The authors construct explicit SL(3,R) black hole solutions, derive their thermodynamics, and demonstrate singularity resolution via gauge transformations, linking the bulk holonomies to boundary CFT data through extended algebras. This work provides a concrete, tractable framework for black hole thermodynamics in theories with extended gauge symmetry and highlights the embedding-dependent relation between geometry and higher spin charges.

Abstract

We investigate higher spin theories of gravity in three dimensions based on the gauge group SL(N,R)*SL(N,R). In these theories the usual diffeomorphism symmetry is enhanced to include higher spin gauge transformations under which traditional geometric notions of curvature and causality are no longer invariant. This implies, for example, that apparently singular geometries can be rendered smooth by a gauge transformation, much like the resolution of orbifold singularities in string theory. The classical solutions, including the recently constructed higher spin black hole, are characterized by their holonomies around the non-contractible cycles of space-time. The black hole solutions are shown to be gauge equivalent to a BTZ black hole which is charged under a set of U(1) Chern-Simons fields. Nevertheless, depending on the choice of embedding of the gravitational gauge group, the space-time geometry may be non-trivial. We study in detail the N=3 example, where this observation allows us to find a gauge where the black hole geometry takes a simple form and the thermodynamic properties can be studied.

Paper Structure

This paper contains 15 sections, 81 equations.