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Chiral $\Lambda$-$\mathfrak{bms}_4$ symmetry of 3d conformal gravity

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arxiv 2405.20244 v3 pith:CM33OKSA submitted 2024-05-30 hep-th gr-qc

classification hep-thgr-qc
keywords algebrachiralmathfrakgravityconformalformalismlambdasymmetry
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abstract

We propose mixed boundary conditions for 3d conformal gravity consistent with variational principle in its second-order formalism that admit the chiral $\Lambda$-$\mathfrak{bms}_4$ algebra as their asymptotic symmetry algebra. This algebra is one of the four chiral $\mathcal W$-algebra extensions of $\mathfrak{so}(2,3)$ and is a generalisation of the chiral $\mathfrak{bms}_4$ algebra responsible for soft theorems of graviton MHV amplitudes in ${\mathbb R}^{1,3}$ gravity to the case of non-zero negative cosmological constant. The corresponding charges calculated using the modified covariant phase space formalism are shown to be finite and integrable, and realise this non-linear ${\cal W}$-algebra.

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  1. Enhanced Conformal $BMS_3$ Symmetries

    hep-th 2024-12 conditional novelty 7.0 of 10

    A boundary-condition analysis of extended conformal gravity in 3D yields a new nonlinear W(2,2,2,2,1,1,1) asymptotic symmetry algebra whose central charges are fixed by the Virasoro central charge.

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