Krylov spread complexity as holographic complexity beyond JT gravity
Michal P. Heller, Jacopo Papalini, Tim Schuhmann
TL;DR
Understanding holographic complexity in black hole interiors remains a central challenge. This work extends the known complexity=volume duality from classical JT gravity to a finite-temperature, fully quantum regime using a duality between double-scaled SYK and sine dilaton gravity. It demonstrates that Krylov spread complexity in DSSYK precisely matches the bulk geodesic length in sine dilaton gravity at finite temperature, valid for all q in (0,1) and all β, by relating length to the boundary Krylov dynamics via the transfer matrix. The authors further identify the first quantum correction to the bulk length as a potential dual to bulk quantum-field Krylov complexity and discuss the switchback effect and future extensions to higher dimensions and non-perturbative completions.
Abstract
One of the important open problems in quantum black hole physics is a dual interpretation of holographic complexity proposals. To date the only quantitative match is the equality between the Krylov spread complexity in triple-scaled SYK at infinite temperature and the complexity = volume proposal in classical JT gravity. Our work utilizes the recent connection between double-scaled SYK and sine-dilaton gravity to show that the quantitative relation between Krylov spread complexity and complexity = volume extends to finite temperatures and to full quantum regime on the gravity side at disk level. From the latter we isolate the first quantum correction to the complexity = volume proposal and propose to view it as a complexity of quantum fields in the bulk. Finally, we comment on the switchback effect, whose presence would make the Krylov spread complexity a fully fledged holographic complexity at least in sine-dilaton gravity.
