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mathcal{N} = (2,2) extended mathfrak{sl}(3|2) Chern-Simons AdS₃ supergravity with new boundaries

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arxiv 2107.11069 v1 pith:KXCWLDP3 submitted 2021-07-23 hep-th gr-qcmath-phmath.MP

mathcal{N} = (2,2) extended mathfrak{sl}(3|2) Chern-Simons AdS₃ supergravity with new boundaries

classification hep-th gr-qcmath-phmath.MP
keywords boundaryconditionsmathcalextendedgeneralsupergravityalgebrasasymptotic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present the first example of $\mathcal{N}=(2,2)$ formulation for the extended higher-spin $AdS_3$ supergravity with the most general boundary conditions as an extension of the $\mathcal{N} =\,(1,1)$ work, discovered recently by us [1]. Using the method proposed by Grumiller and Riegler, we construct a consistent class of the most general boundary conditions to extend it. An important consequence of our method is that, for the loosest set of boundary conditions it ensures that their asymptotic symmetry algebras consist of two copies of the $\mathfrak{sl}(3|2)_k$. Moreover, we enjoin some certain restrictions on the gauge fields for the most general boundary conditions, leading to the supersymmetric extensions of the Brown and Henneaux boundary conditions. Based on these results, we finally find out that the asymptotic symmetry algebras are two copies of the super $\mathcal{W}_3$ algebra for $\mathcal{N} = (2,2)$ extended higher-spin supergravity theory in $AdS_3$.

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Cited by 2 Pith papers

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  1. Generalized Schwarzian Dynamics from a Bulk-First BF Perspective

    hep-th 2026-06 unverdicted novelty 5.5

    Generalized Schwarzian dynamics, including sl(3,R) Wilczynski invariants, arise as reduced boundary dynamics of flat BF connections rather than as an independent boundary theory.

  2. Generalized Schwarzian Dynamics from a Bulk-First BF Perspective

    hep-th 2026-06 conditional novelty 4.0

    The sl(3,R) BF reduction is re-expressed through Wilczynski invariants, yielding a generalized Schwarzian action and a heuristic thermodynamic dictionary to Casimir and monodromy data.