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Accelerating Black Holes in 2+1 dimensions: Holography revisited

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arxiv 2308.00613 v2 pith:CVLCH5CZ submitted 2023-08-01 hep-th gr-qc

Accelerating Black Holes in 2+1 dimensions: Holography revisited

classification hep-th gr-qc
keywords holographicacceleratingaccelerationactionblackboundarycomputeentanglement
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This paper studies the holographic description of $2+1-$dimensional accelerating black holes. We start by using an ADM decomposition of the coordinates suitable to identify boundary data. As a consequence, the holographic CFT lies in a fixed curved background which is described by the holographic stress tensor of a perfect fluid. We compute the Euclidean action ensuring that the variational principle is satisfied in the presence of the domain wall. This requires including the Gibbons--Hawking--York term associated with internal boundaries on top of the standard renormalised AdS$_{3}$ action. Finally, we compute the entanglement entropy by firstly mapping the solution to the Rindler--AdS spacetime in which the Ryu--Takayanagi surface is easily identifiable. We found that as the acceleration increases the accessible region of the conformal boundary decreases and also the entanglement entropy, indicating a loss of information in the dual theory due to acceleration.

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Cited by 2 Pith papers

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  1. Decoupling Limit of Quiver Theories and the Angular Spectra of Extreme C-metrics

    hep-th 2026-07 conditional novelty 6.0

    Angular eigenvalues of the extreme charged C-metric are computed analytically via a confluent limit of SU(2)×SU(2) quiver gauge theory, matching numerical results.

  2. Radiation in Fluid/Gravity and the Flat Limit

    hep-th 2025-08 unverdicted novelty 6.0

    Establishes a holographic link between bulk gravitational radiation and dissipative corrections plus entropy production in boundary fluids, then constructs Carrollian analogues and celestial observables in the flat limit.