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Complexity Near Horizons

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.

3 nodes2 linksoverview mapComplexity Near Horizons
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Complexity Near Horizons3 visible / 3 total nodes / 2 links
AuthorshipTopic signalWComplexity Near Horizonspreprint / 2015AEdi HalyoResearcherThep-th13268 works
PaperSignal 102 links

Complexity Near Horizons

preprint / 2015

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