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Holographic complexity of rotating black holes

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arxiv 2010.11203 v3 pith:JNUL3PFT submitted 2020-10-21 hep-th gr-qc

Holographic complexity of rotating black holes

classification hep-th gr-qc
keywords complexityblackholesequalsformationholographicrotatingvolume
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Within the framework of the "complexity equals action" and "complexity equals volume" conjectures, we study the properties of holographic complexity for rotating black holes. We focus on a class of odd-dimensional equal-spinning black holes for which considerable simplification occurs. We study the complexity of formation, uncovering a direct connection between complexity of formation and thermodynamic volume for large black holes. We consider also the growth-rate of complexity, finding that at late-times the rate of growth approaches a constant, but that Lloyd's bound is generically violated.

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Cited by 2 Pith papers

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

  1. Holographic complexity of de-Sitter black holes

    hep-th 2026-06 unverdicted novelty 5.0

    In SdS black hole holography, CV and CV2.0 complexities grow linearly while CA growth vanishes due to finite action, with matching rates between static patch and dS/CFT schemes.

  2. A Timelike Quantum Focusing Conjecture

    hep-th 2026-04 unverdicted novelty 5.0

    A timelike quantum focusing conjecture implies a complexity-based quantum strong energy condition and a complexity bound analogous to the covariant entropy bound for suitable codimension-0 field theory complexity measures.