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arXiv · 2001.06453

Action Complexity for Semi-Classical Black Holes

Lukas Schneiderbauer·Watse Sybesma·Lárus Thorlacius
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Abstract

We adapt the complexity as action prescription (CA) to a semi-classical model of two-dimensional dilaton gravity and determine the rate of increase of holographic complexity for an evaporating black hole. The results are consistent with our previous numerical results for semi-classical black hole complexity using a volume prescription (CV) in the same model, but the CA calculation is fully analytic and provides a non-trivial positive test for the holographic representation of the black hole interior.

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Lukas Schneiderbauer, Watse Sybesma, Lárus Thorlacius. 2020-01-17. Action Complexity for Semi-Classical Black Holes. https://doi.org/10.1007/jhep07(2020)173

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