Abstract

In this work, we consider non-linear corrections to the Langevin effective theory of a heavy quark moving through a strongly coupled CFT plasma. In AdS/CFT, this system can be identified with that of a string stretched between the boundary and the horizon of an asymptotically AdS black brane solution. We compute the Feynman-Vernon influence phase for the heavy quark by evaluating the Nambu-Goto action on a doubled string configuration. This configuration is the linearised solution of the string motion in the doubled black brane geometry which has been proposed as the holographic dual of a thermal Schwinger-Keldysh contour of the CFT. Our expression for the influence phase passes non-trivial consistency conditions arising from the underlying unitarity and thermality of the bath. The local effective theory obeys the recently proposed non-linear fluctuation dissipation theorem relating the non-Gaussianity of thermal noise to the thermal jitter in the damping constant. This furnishes a non-trivial check for the validity of these relations derived in the weak coupling regime.

Highlights

  • Non-linear Langevin theoryOur goal is to introduce the non-linear Langevin theory for the Brownian particle and its description within Schwinger-Keldysh formalism

  • The classic result of fluctuation dissipation theorem asserts that this variance of the fluctuation f 2 is directly proportional to the coefficient of linear drag/dissipation γ

  • On examining the influence phase computed from the string configuration, we find that the universal non-linear Langevin dynamics derived from weakly coupled intuition, continues to describe the non-linearities in this strongly coupled system

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Summary

Non-linear Langevin theory

Our goal is to introduce the non-linear Langevin theory for the Brownian particle and its description within Schwinger-Keldysh formalism. We are interested in a heavy quark coupled to a CFTd plasma at a temperature T This quark feels a variety of forces, which at a macroscopic effective theory level result in energy/momentum dissipation and fluctuations. We immediately note that the system under consideration has a variety of symmetries including translational, rotational and reflection invariance These symmetries drastically reduce the number of non-linear corrections to the linear theory that can appear in general. The non-linear Langevin dynamics described by eq (2.1) will be shown to be dual to a Schwinger-Keldysh effective theory. We will argue that the ζγ-term in this equation represents the universal leading correction (consistent with the symmetries) to the standard linear Langevin dynamics

Stochastic path integral
Heavy quark in SK formalism
Holographic Brownian motion
The black brane and the holographic SK contour
The Nambu-Goto action
Ingoing quasi-normal modes
Outgoing Hawking modes
The doubled string on holographic SK contour
Influence phase of the heavy quark
Influence phase in Keldysh basis and its derivative expansion
Discussion and conclusion
Retarded bulk to boundary Green’s function
B Exact solution in AdS3
Full Text
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