Abstract

Quantum fields with large degeneracy are often approximated as classical fields. Here, we show how quantum and classical evolution of a highly degenerate quantum field with repulsive contact self-interactions differ from each other. Initially, the field is taken to be homogeneous except for a small plane wave perturbations in only one mode. In quantum field theory, modes satisfying both momentum and energy conservation of the quasi-particles, grow exponentially with time. However, in the classical field approximation, the system is stable. We calculate the time scale after which the classical field description becomes invalid.

Highlights

  • The duration of classicality tcl is the longest time for which the dynamics of a quantum system can be accurately approximated by the dynamics of an analogous classical system

  • This work was motivated by the following question: how long can a highly degenerate quantum scalar field be accurately described by classical field equations? Intuitively, this time scale cannot be longer than the thermalization time scale

  • A generic formalism to calculate the duration of classicality was developed in Ref. [4]

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Summary

INTRODUCTION

The duration of classicality tcl is the longest time for which the dynamics of a quantum system can be accurately approximated by the dynamics of an analogous classical system. One could choose initial conditions such that hN jð0Þi ≈ Njð0Þ, and trust that the quantum and classical equations will make similar predictions for an indefinitely long time, up to small corrections. Λljmk 1⁄4 0, these differences are not relevant, as both equations are linear and the operators ajðtÞ and the amplitudes AjðtÞ have the same time dependence This implies that, if hN jðtÞi 1⁄4 NjðtÞ initially, it will always be so. [4], the quantum treatment of the initial time evolution of homogeneous fields was given for the cases of attractive contact interactions and for gravitational self-interactions In both cases, an estimate for tcl was provided. III, we solve the linearized Heisenberg equations of motion and obtain an analytical expression for tcl

CLASSICAL BEHAVIOR
One-mode inhomogeneity
Higher-order corrections
QUANTUM CORRECTIONS
Duration of classicality
QðΛÞδωðjδnn0jÞ ln
SUMMARY AND CONCLUSIONS
16 Λ3ðΛ2 þ
Full Text
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