Complexity Near Horizons
High Energy Physics - Theory
2015-06-23 v1
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 during proper time which corresponds to the creation of a causal patch with proper length inside the horizon. We attempt to describe complexity in the horizon CFT and the Euclidean picture.
Keywords
Cite
@article{arxiv.1506.06611,
title = {Complexity Near Horizons},
author = {Edi Halyo},
journal= {arXiv preprint arXiv:1506.06611},
year = {2015}
}
Comments
15 pages