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Effects of the acceleration on holographic complexity

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arxiv 2205.00196 v2 pith:RGTPXA65 submitted 2022-04-30 hep-th

classification hep-th
keywords blackaccelerationholeskindstringworkconsidereffect
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In this work we consider a spacial kind of spacetime called AdS accelerating black holes. This is a kind of black holes which contain a stringlike singularity along polar axises attached to the black hole and it accelerates the black hole. In these kind of spacetimes the growth of Einstein-Hilbert action is independent of the acceleration as found in the previous works. By using a string as a probe, we found the effect of the acceleration is captured by the string prove in our previous work. Here in this work we consider the case of rotating black holes. By the prove string we clearly describe the effect of the acceleration and its relation to the rotation of the black holes.

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  1. $R^2$ corrections to Complexity Growth with a Probe String

    hep-ph 2025-07 conditional novelty 4.0 of 10

    In Gauss-Bonnet AdS5, the probe-string complexity growth is maximized at zero velocity, independent of the GB coupling when stationary, and linear in temperature.

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