Brownian motion in AdS/CFT

TL;DR

This paper models Brownian motion of a quark in a strongly coupled plasma using AdS/CFT, deriving the Langevin equation from string dynamics in a black hole background and exploring related black hole horizon properties.

Contribution

It provides a bulk derivation of the Langevin equation for a Brownian particle in AdS/CFT and connects string excitations to boundary stochastic dynamics.

Findings

Derived the Langevin equation from string dynamics in AdS black hole backgrounds.

Established the fluctuation-dissipation theorem in the holographic context.

Explored the membrane paradigm and horizon properties related to Brownian motion.

Abstract

We study Brownian motion and the associated Langevin equation in AdS/CFT. The Brownian particle is realized in the bulk spacetime as a probe fundamental string in an asymptotically AdS black hole background, stretching between the AdS boundary and the horizon. The modes on the string are excited by the thermal black hole environment and consequently the string endpoint at the boundary undergoes an erratic motion, which is identified with an external quark in the boundary CFT exhibiting Brownian motion. Semiclassically, the modes on the string are thermally excited due to Hawking radiation, which translates into the random force appearing in the boundary Langevin equation, while the friction in the Langevin equation corresponds to the excitation on the string being absorbed by the black hole. We give a bulk proof of the fluctuation-dissipation theorem relating the random force and friction. This work can be regarded as a step toward understanding the quantum microphysics underlying the fluid-gravity correspondence. We also initiate a study of the properties of the effective membrane or stretched horizon picture of black holes using our bulk description of Brownian motion.