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Nonequilibrium Green Functions and Kadanoff–Baym Evolution

Nonequilibrium Green-function theory evolves correlations at two independent times. It is therefore more general than a Boltzmann equation, but also more demanding: a result is meaningful only after the self-energy closure, initial correlations, renormalization, memory treatment, spectral normalization, and numerical convergence have all been exposed. This chapter develops that chain without assuming quasiparticles or time-translation invariance.

From exact two-time identities to controlled reductions

Section titled “From exact two-time identities to controlled reductions”

Start with two-time Green functions and self-energies to separate local mass terms from nonlocal collision kernels. 2PI effective actions then provide self-consistent closures and a precise, limited conservation theorem. The Kadanoff–Baym equations turn the contour Dyson equation into causal initial-value equations for the statistical and spectral correlators.

The remaining pages each test one reduction or input:

Reading routes through two-time nonequilibrium evolution
Question Start with Necessary check Stop condition
What is being evolved? Two-time functions Contour, sign, and equal-time conventions Do not Fourier transform in relative time before approximate stationarity is demonstrated.
Is the closure conserving? 2PI truncations Invariant functional and renormalized stationary equation Conservation alone does not establish Ward identities, gauge independence, crossing, or accuracy.
Can memory be reduced? Memory and Wigner pages Correlation-time and gradient studies Long tails, narrow widths, finite-time edges, or rapid phases invalidate a local kinetic reduction.
Is the computation trustworthy? Numerical validation Independent step, grid, cutoff, memory, and truncation studies A smooth curve or small solver residual is not a continuum or closure test.

For a real scalar field this chapter uses

F(x,y)=12{ϕ(x),ϕ(y)},ρ(x,y)=i[ϕ(x),ϕ(y)].F(x,y)=\frac12\langle\{\phi(x),\phi(y)\}\rangle, \qquad \rho(x,y)=i\langle[\phi(x),\phi(y)]\rangle .

Thus F(y,x)=F(x,y)F(y,x)=F(x,y), ρ(y,x)=ρ(x,y)\rho(y,x)=-\rho(x,y), and canonical normalization gives ρ(t,t)=0\rho(t,t)=0 and tρ(t,t)t=t=1\partial_t\rho(t,t')|_{t=t'}=1 mode by mode. Other sign conventions are common; importing an equation without transforming all propagators, self-energies, and boundary conditions is a frequent source of wrong signs. Spatial homogeneity is introduced only in checked examples, not in the formal derivations.

The chapter treats closed-system two-point evolution. Open-system influence kernels, stochastic unravellings, gauge-covariant kinetic theory, and downstream phenomenology require additional assumptions and are not consequences of a two-time solution alone.

  • Baym, G. (1962). “Self-Consistent Approximations in Many-Body Systems.” Physical Review 127, 1391–1401. DOI.
  • Berges, J. (2004). “Introduction to Nonequilibrium Quantum Field Theory.” AIP Conference Proceedings 739, 3–62. arXiv:hep-ph/0409233; DOI.
  • Kadanoff, L. P., and Baym, G. (1962). Quantum Statistical Mechanics. New York: W. A. Benjamin. Internet Archive record.