Replica evolution of classical field in 4+1 dimensional spacetime toward real time dynamics of quantum field

TL;DR

This paper proposes a replica-based classical field evolution method in 4+1 dimensions to approximate real-time quantum dynamics at finite temperatures, demonstrating its effectiveness in quantum mechanics and scalar field theory.

Contribution

It introduces a novel replica evolution approach that connects classical simulation techniques with quantum field dynamics, including divergence removal and thermal mass behavior.

Findings

Replica evolution reproduces quantum equilibrium distribution.

Accurately describes unequal-time correlations in harmonic oscillator.

Thermal mass growth matches perturbative estimates in small coupling.

Abstract

Real-time evolution of replicas of classical field is proposed as an approximate simulator of real-time quantum field dynamics at finite temperatures. We consider $N$ classical field configurations dubbed as replicas which interact with each other via the $\tau$-derivative terms and evolve with the classical equation of motion. The partition function of replicas is found to be proportional to that of quantum field in the imaginary time formalism. As the replica index $\tau$ can be regarded as the imaginary time index, the replica evolution is technically the same as the molecular dynamics part of the hybrid Monte-Carlo sampling and the replica configurations should reproduce the correct quantum equilibrium distribution after the long-time evolution. At the same time, evolution of the replica-index average of field variables is described by the classical equation of motion when the fluctuations are small. In order to examine the real-time propagation properties of replicas, we first discuss replica evolution in quantum mechanics. Statistical averages of observables are precisely obtained by the initial condition average of replica evolution, and the time evolution of the unequal-time correlation function, $\langle x(t) x(t')\rangle$, in a harmonic oscillator is also described well by the replica evolution in the range $T/\omega > 0.5$. Next, we examine the statistical and dynamical properties of the $\phi^4$ theory in the 4+1 dimensional spacetime, which contains three spatial, one replica index or the imaginary time, and one real-time. We note that the Rayleigh-Jeans divergence can be removed in replica evolution with $N \geq 2$ when the mass counterterm is taken into account. We also find that the thermal mass obtained from the unequal-time correlation function at zero momentum grows as a function of the coupling as in the perturbative estimate in the small coupling region.