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Holographic Complexity and Thermodynamic Volume

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arxiv 2008.09138 v1 pith:GCULYZBQ submitted 2020-08-20 hep-th gr-qc

classification hep-thgr-qc
keywords complexityvolumethermodynamicblackentropyformationholesequals
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We study the holographic complexity conjectures for rotating black holes, uncovering a relationship between the complexity of formation and the thermodynamic volume of the black hole. We suggest that it is the thermodynamic volume and not the entropy that controls the complexity of formation of large black holes in both the Complexity Equals Action and Complexity Equals Volume proposals in general. Our proposal reduces to known results involving the entropy in settings where the thermodynamic volume and entropy are not independent, but has broader scope. Assuming a conjectured inequality is obeyed by the thermodynamic volume, we establish that the complexity of formation is bounded from below by the entropy for large black holes.

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Cited by 1 Pith paper

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  1. Thermodynamics of charged rotating black strings in extended phase space

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Charged rotating AdS black strings show a specific-heat divergence that is interpreted as a second-order, Van der Waals-like critical point, while uncharged strings show no such criticality.

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