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Asymptotic structure of three-dimensional Maxwell Chern-Simons gravity coupled to spin-3 fields

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arxiv 2412.04992 v1 pith:GS2Z4WG7 submitted 2024-12-06 hep-th gr-qc

classification hep-thgr-qc
keywords algebramathfrakasymptoticgravitymaxwellchern-simonsextensionsymmetries
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abstract

In this work we analyze the asymptotic symmetries of the three-dimensional Chern-Simons (CS) gravity theory for a higher spin extension of the so-called Maxwell algebra. We propose a generalized set of asymptotic boundary conditions for the aforementioned flat gravity theory and we show that the corresponding charge algebra defines a higher-spin extension of the $\mathfrak{max}$-$\mathfrak{bms}_{3}$ algebra, which in turn corresponds the asymptotic symmetries of the Maxwell CS gravity. We also show that the $\mathfrak{hs}_3\mathfrak{max}$-$\mathfrak{bms}_{3}$ algebra can alternatively be obtained as a vanishing cosmological constant limit of three copies of the $\mathcal{W}_3$ algebra, with three independent central charges.

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  1. Boundary dynamics of Maxwell-invariant three-dimensional Chern-Simons gravity

    hep-th 2025-06 conditional novelty 5.0 of 10

    A Maxwellian extension of flat Liouville theory is derived as the boundary dual of Maxwell-invariant 2+1 Chern-Simons gravity, and is shown to match a geometric action and a Carrollian expansion of the AdS3 dual.

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