On the time dependence of holographic complexity for charged AdS black holes with scalar hair
Roberto Auzzi, Stefano Bolognesi, Eliezer Rabinovici, Fidel I., Schaposnik Massolo, Gianni Tallarita

TL;DR
This paper investigates how holographic complexity evolves over time in charged AdS black holes with scalar hair, revealing that volume complexity respects the Lloyd bound while action complexity diverges at critical times but remains bounded asymptotically.
Contribution
It provides a detailed analysis of the time dependence of holographic complexity in hairy black holes, highlighting differences between volume and action proposals and their relation to the Lloyd bound.
Findings
Volume complexity respects the Lloyd bound across parameters.
Action complexity diverges at a critical time when the WDW patch touches the singularity.
Asymptotic action complexity rate satisfies the Lloyd bound.
Abstract
In the presence of a scalar hair perturbation, the Cauchy horizon of a Reissner-Nordstr\"om black hole disappears and is replaced by the rapid collapse of the Einstein-Rosen bridge, which leads to a Kasner singularity [1,2]. We study the time-dependence of holographic complexity, both for the volume and for the action proposals, in a class of models with hairy black holes. Volume complexity can only probe a portion of the black hole interior that remains far away from the Kasner singularity. We provide numerical evidence that the Lloyd bound is satisfied by the volume complexity rate in all the parameter space that we explored. Action complexity can instead probe a portion of the spacetime closer to the singularity. In particular, the complexity rate diverges at the critical time for which the Wheeler-DeWitt patch touches the singularity. After the critical time the action…
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