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/ which corresponds to the creation of a causal patch with proper length 1/ inside the horizon. We attempt to describe complexity in the horizon CFT and the Euclidean picture.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.