Complexity Near Horizons

Abstract

We generalize the concept of complexity near horizons to all nondegenerate black holes. For Schwarzschild black holes, we show that Rindler observers see a complexity change of $S$ during proper time $1/\kappa$ which corresponds to the creation of a causal patch with proper length $1/\kappa$ inside the horizon. We attempt to describe complexity in the horizon CFT and the Euclidean picture.

15 pages

References in corpus (6)

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• Horizon Conformal Field Theories from $Ad{S}_2$ Black Holes
• Rindler Energy is Wald Entropy
• On the Holographic Nature Of Rindler Energy