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Localised $\bf{AdS_5\times S^5}$ Black Holes

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arxiv 1605.04911 v1 pith:NRR4PRP6 submitted 2016-05-16 hep-th gr-qc

classification hep-thgr-qc
keywords mathrmphasetimestransitionblackenergiesholeslocalised
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We numerically construct asymptotically global $\mathrm{AdS}_5\times \mathrm{S}^5$ black holes that are localised on the $\mathrm{S}^5$. These are solutions to type IIB supergravity with $\mathrm S^8$ horizon topology that dominate the theory in the microcanonical ensemble at small energies. At higher energies, there is a first-order phase transition to $\mathrm{AdS}_5$-Schwarzschild$\times \mathrm{S}^5$. By the AdS/CFT correspondence, this transition is dual to spontaneously breaking the $SO(6)$ R-symmetry of $\mathcal N=4$ super Yang-Mills down to $SO(5)$. We extrapolate the location of this phase transition and compute the expectation value of the resulting scalar operators in the low energy phase.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Charged Rotating Hairy Black Holes in AdS$_5 \times S^5$: Unveiling their Secrets

    hep-th 2024-11 conditional novelty 7.0 of 10

    The BPS limit of the newly constructed hairy black holes has zero entropy and a diverging scalar field, so no regular supersymmetric hairy black holes exist in this sector.

  2. Holographic Timelike Entanglement and Subregion Complexity in Localized AdS3*S3*T4 Black Holes

    hep-th 2026-07 conditional novelty 6.0 of 10

    Timelike entanglement and subregion complexity detect the cap–horizon transition of localized AdS3×S3×T4 black poles via fixed-boundary-interval Lorentzian branch selection, effects absent in BTZ and large-r limits.

  3. A Reverse Black Hole Information Problem

    hep-th 2026-01 conditional novelty 6.0 of 10

    Exact CFT states for colliding particles that form evaporating AdS black holes are constructed, and several coarse-graining maps are shown to convert the exact pure state into mixed semiclassical Hawking radiation wit...

  4. Localized Black Holes in AdS$_3$: What Happens Below c/12 Stays Below c/12

    hep-th 2024-12 conditional novelty 6.0 of 10

    Localized black holes in AdS3 x S3 x T4 fill the low-energy spectrum, dominate the microcanonical ensemble below a small positive energy, and appear to have the same entanglement entropy as BTZ black holes.

  5. A Central Charge for sub-AdS Holography

    hep-th 2024-12 conditional novelty 5.0 of 10

    Sub-AdS scales are mapped to sub-stacks of M < N D-branes, yielding a scale-dependent central charge c(R0) = (R0/L)^{d+q-1} c(L), with consistency checks from small black holes and Dp-brane theories.

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