Holographic Krylov complexity for Yang-Baxter deformed supergravity backgrounds
Dibakar Roychowdhury

TL;DR
This paper calculates holographic Krylov complexity for strongly coupled quantum field theories dual to Yang-Baxter deformed supergravity backgrounds, revealing how deformations influence complexity growth.
Contribution
It introduces a method to compute Krylov complexity in YB deformed backgrounds and analyzes the deformation's impact on complexity growth rates.
Findings
YB deformation affects the bulk momentum of particles
Complexity growth rate varies with YB parameter
Results recover the undeformed case when YB parameter approaches zero
Abstract
We compute the holographic Krylov complexity for a class of strongly coupled QFTs in a top down approach, where the dual gravitational counterpart corresponds to Yang-Baxter (YB) deformed supergravity solutions in a type IIB set up. The full 10d solution contains the as the subspace, along with the dilaton and the background RR and NS fluxes. The Krylov complexity in the dual operator picture is obtained by computing the proper momentum of the massive particle along its geodesic in the bulk spacetime. We explore the effects of YB deformation on the bulk momentum of the particle, which in turn affects the rate of growth of complexity in the dual QFTs. Our results boil down into the undeformed case in the appropriate limit of the YB parameter.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Geometry and complex manifolds · Quantum Chromodynamics and Particle Interactions
