Complexity Near Horizons

Edi Halyo

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arXiv · 1506.06611

Complexity Near Horizons

Edi Halyo

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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 $1/κ$ which corresponds to the creation of a causal patch with proper length $1/κ$ inside the horizon. We attempt to describe complexity in the horizon CFT and the Euclidean picture.

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Edi Halyo. 2015-06-22. Complexity Near Horizons. https://arxiv.org/abs/1506.06611

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