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Holographic Complexity of Einstein-Maxwell-Dilaton Gravity

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arxiv 1712.09826 v2 pith:PVCFFXKW submitted 2017-12-28 hep-th cond-mat.stat-mechquant-ph

Holographic Complexity of Einstein-Maxwell-Dilaton Gravity

classification hep-th cond-mat.stat-mechquant-ph
keywords complexityactiongrowthhyperscalingeinstein-maxwell-dilatongravityholographicaspects
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the holographic complexity of Einstein-Maxwell-Dilaton gravity using the recently proposed "complexity = volume" and "complexity = action" dualities. The model we consider has a ground state that is represented in the bulk via a so-called hyperscaling violating geometry. We calculate the action growth of the Wheeler-DeWitt patch of the corresponding black hole solution at non-zero temperature and find that, in the presence of violations of hyperscaling, there is a parametric enhancement of the action growth rate. We partially match this behavior to simple tensor network models which can capture aspects of hyperscaling violation. We also exhibit the switchback effect in complexity growth using shockwave geometries and comment on a subtlety of our action calculations when the metric is discontinuous at a null surface.

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Cited by 2 Pith papers

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  2. Holographic complexity of de-Sitter black holes

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    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.