Abstract

We analytically calculate the perturbation expansion of the two-point correlation function (propagator) of the scalar, dissipative quantum ${\ensuremath{\varphi}}^{4}$ theory up to third order in the interaction parameter $\ensuremath{\lambda}$. The calculations are carried out with two different methods. The first is based on a brute force computation of all interactions appearing in the perturbation expansion term by term at the given order of the perturbation, supported by the use of a symbolic mathematical code. The second uses an efficient perturbation scheme which allows one to hierarchically organize terms within a given order in the perturbation expansion based on the number of occurrences of the free evolution operator ${\mathcal{R}}_{s}^{\mathrm{free}}$; in addition, it allows one to utilize information from already computed lower-order terms in the calculation of higher-order terms. The two methods yield the same result. In the limit of zero dissipation (zero friction coefficient $\ensuremath{\gamma}$), our result coincides with that obtained from the Lagrangian approach in $D=d+1$ dimensions ($d$ denotes the number of space dimensions, while $D$ includes the time dimension) with the use of $D$-dimensional vectors, re-expressed in terms of only $d$-dimensional space integrals by integrating out the zero component. We have also verified that the value of the critical coupling constant ${\ensuremath{\lambda}}^{*}$ as a function of space dimensionality $d$, which can be used to evaluate perturbation expansions at the physical length scale ${\ensuremath{\ell}}_{m}$, comes out correctly from our third-order calculation.

Highlights

  • In quantum field theories, Feynman diagrams involving closed loops require integration over all possible combinations of energy and momentum of the virtual particles traveling around the loop and are often divergent

  • Behind renormalization is the problem of the proper, successive elimination of degrees of freedom in the effort to bridge a wide range of length scales and, in relativistic quantum field theory, clearly of time scales [4,5,6]

  • Considering irreversibility to be an intrinsic feature of any quantum field theory, since the divergences arise from spontaneous particle creation and annihilation

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Summary

INTRODUCTION

Feynman diagrams involving closed loops require integration over all possible combinations of energy and momentum of the virtual particles traveling around the loop and are often divergent. The quantum master equation describes collisions of free particles (field quanta) as well as the interaction with a heat bath representing small-scale features. The dissipative coupling to the heat bath in the thermodynamic quantum master equation provides a proper highenergy (ultraviolet) cutoff, a regularization of the theory for dynamic properties. The first includes two fields and serves to define the propagator, while the second includes four fields and corresponds to the effective interaction vertex The latter has helped [4] compute the fixed point value of the dimensionless coupling constant [3]. We apply the dissipative quantum field theory [4] to calculate the two-point correlation function (propagator) of the scalar φ4 theory up to third order in the interaction parameter λ.

DISSIPATIVE SCALAR FIELD THEORY
THE PROPAGATOR UP TO THIRD ORDER
Zeroth-order propagator
First-order propagator
Second-order propagator
LIMIT OF VANISHING DISSIPATION
REGULARIZATION
CALCULATION OF λÃ
48 Z 128ð2πÞd ddk1
SUMMARY AND DISCUSSION

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