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Shockwaves in black hole microstate geometries

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arxiv 2112.08378 v2 pith:XB2RHHY6 submitted 2021-12-15 hep-th gr-qc

classification hep-thgr-qc
keywords blackholeshockwavessolutionsmicrostatefamilymicrostatessupersymmetric
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Gravitational solutions involving shockwaves have attracted significant recent interest in the context of black holes and quantum chaos. Certain classes of supersymmetric two-charge black hole microstates are described by supergravity solutions containing shockwaves, that are horizonless and smooth away from the shockwave. These configurations have been used to describe how black hole microstates absorb and scramble perturbations. In this paper we construct the first family of asymptotically flat supersymmetric three-charge microstate solutions that contain shockwaves. We identify a family of holographically dual states of the D1-D5 CFT and show that these pass a set of tests, including a precision holographic test. We find precise agreement between gravity and CFT. Our results may prove useful for constructing more general families of black hole microstate solutions.

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  1. Cogito, ergo - strings: Supersymmetric ergoregions and their stringy excitations

    hep-th 2025-08 unverdicted novelty 6.0 of 10

    Supersymmetric ergoregions without horizons in NS5-F1-P bound states are shown to admit negative-energy BPS excitations, described via gauged WZW models and mapped holographically to the dual CFT.

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