Abstract

We review the Schwinger-Keldysh, or in-in, formalism for studying quantum dynamics of systems out-of-equilibrium. The main motivation is to rephrase well known facts in the subject in a mathematically elegant setting, by exhibiting a set of BRST symmetries inherent in the construction. We show how these fundamental symmetries can be made manifest by working in a superspace formalism. We argue that this rephrasing is extremely efficacious in understanding low energy dynamics following the usual renormalization group approach, for the BRST symmetries are robust under integrating out degrees of freedom. In addition we discuss potential generalizations of the formalism that allow us to compute out-of-time-order correlation functions that have been the focus of recent attention in the context of chaos and scrambling. We also outline a set of problems ranging from stochastic dynamics, hydrodynamics, dynamics of entanglement in QFTs, and the physics of black holes and cosmology, where we believe this framework could play a crucial role in demystifying various confusions. Our companion paper [1] describes in greater detail the mathematical framework embodying the topological symmetries we uncover here.

Highlights

  • The study of quantum dynamics out of equilibrium and in open systems necessarily involves working with mixed states

  • We review the Schwinger-Keldysh, or in-in, formalism for studying quantum dynamics of systems out-of-equilibrium

  • We argue that this rephrasing is extremely efficacious in understanding low energy dynamics following the usual renormalization group approach, for the BRST symmetries are robust under integrating out degrees of freedom

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Summary

Introduction

The study of quantum dynamics out of equilibrium and in open systems necessarily involves working with mixed states. Our motivation for getting intrigued by the problem of constructing effective Schwinger-Keldysh theories was primarily to understand the general structure of such effective actions in the fluid dynamical regime and beyond [9, 12].2 These are qualitatively similar to the classic problem of the Brownian oscillator which motivated [2], or linear dissipative systems which inspired [4], albeit with a necessary upgrade to non-Gaussian interactions. Understanding the emergence of this gauge symmetry led us to revisiting the essentials of the Schwinger-Keldysh formalism, which as we outlined in [9] are best viewed by extracting the topological invariances inherent in the construction This suffices to reproduce the effective actions of [12, 21] for fluid dynamics as we recently explained in [22].4.

A lighting review of standard Schwinger-Keldysh formalism
The basics of the Schwinger-Keldysh formalism
Schwinger-Keldysh time ordering
Step function conventions
Keldysh basis correlators
SK causality
Thermal correlation functions in Schwinger-Keldysh formalism
Thermal equilibrium in stationary curved spacetimes
The KMS condition
Thermal sum rules from KMS
The retarded-advanced basis
Retarded-advanced correlators
The thermofield double
Examples
Free scalar field
Free fermion field
Vector field
BRST symmetries and ghosts
Field redefinition BRST symmetries
The topological sector of Schwinger-Keldysh
SK supercharges
Example: free scalar field
The Schwinger-Keldysh superfields
Thermal BRST symmetries and SK-KMS superalgebra
The KMS supercharges
The quadruplet of thermal translations
SK-KMS superalgebra in superspace
Thermal equivariant cohomology
Physical origins of the supercharges
CPT symmetries
Superspace Keldysh rules
Two-point functions A generic superfield two-point function reads
10 Timefolds and out-of-time-order observables
11 Applications to physical problems
Full Text
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