Time Evolution of Complexity in Abelian Gauge Theories - And Playing Quantum Othello Game -
Koji Hashimoto, Norihiro Iizuka, Sotaro Sugishita
TL;DR
This work probes how quantum complexity evolves in Abelian gauge theories by discretizing U(1) to Z_N on a lattice and defining a universal gate set. It shows that achieving exponential-in-entropy complexity requires maximally nonlocal Hamiltonians, linking nonlocality to potential gravity duals, and demonstrates how locality constraints suppress the maximum attainable complexity. Through both classical random-flux models and fully quantum analyses, the paper characterizes how complexity grows and saturates, and how nonlocal interactions (embodied by Othello/CNOT-like gates) accelerate growth. The results illuminate when gauge theories may replicate the fast information processing associated with black holes and provide a framework for comparing locality, entanglement, and complexity in gauge/gravity duality contexts.
Abstract
Quantum complexity is conjectured to probe inside of black hole horizons (or wormhole) via gauge gravity correspondence. In order to have a better understanding of this correspondence, we study time evolutions of complexities for generic Abelian pure gauge theories. For this purpose, we discretize $U(1)$ gauge group as $\mathbf{Z}_N$ and also continuum spacetime as lattice spacetime, and this enables us to define a universal gate set for these gauge theories, and evaluate time evolutions of the complexities explicitly. We find that for a generic class of diagonal Hamiltonians to achieve a large complexity $\sim \exp(\mbox{entropy})$, which is one of the conjectured criteria necessary to have a dual black hole, the Abelian gauge theory needs to be maximally nonlocal.
