Skip to content

Many-body quantum mechanics already uses quantum fields: creation operators, collective modes, and local correlations are field-theory objects. To continue, choose the question you want to answer. A path integral, a critical exponent, a thermal spectrum, and a diffusion coefficient require different additional tools.

The QFT library develops these tools in connected subject volumes. The links below lead to its current volume pages, where you can choose the relevant chapter.

Helpful background. The many-body QFT bridge overview explains how field operators, functional integrals, and collective variables fit together.

Quantum Field Theory Routes from a Many-Body Problem

Section titled “Quantum Field Theory Routes from a Many-Body Problem”

Start with many-body path integrals and coherent-state path integrals if you need a partition function, a source derivative, or an effective action. Be able to identify the measure, time ordering, boundary conditions, and operator represented by a source.

Continue to Foundations of Quantum Field Theory, especially its functional-integral and correlator chapters. These develop regulated Gaussian fields, connected correlators, and the one-particle-irreducible effective action. A formula such as Z[J]=∫Dϕ eiS+i∫JϕZ[J]=\int\mathcal D\phi\,e^{iS+i\int J\phi} is shorthand for that regulated construction, not a definition independent of its state and boundary prescription.

Use nonrelativistic fields and many-body Green functions to connect a particle Hamiltonian to densities, spectra, and response. Fixed particle number remains a possible sector of the field theory.

Many-Body QFT and Quantum Matter continues toward interacting fields and collective descriptions. Relativity, antiparticles, and dynamical gauge fields are additional physical ingredients when appropriate; nonrelativistic quantum field theory is already QFT.

Work through statistical field theory and the criticality bridge when microscopic parameters appear to disappear from a long-distance answer.

Renormalization and Effective Field Theory explains regulator dependence, running couplings, operator mixing, and matching. The practical question is which measurements stay fixed as the cutoff changes. An irrelevant coupling may still be needed to interpret an observable, and a relevant perturbation need not always produce a gapped phase.

The thermal QFT bridge relates the Gibbs trace, Matsubara functions, and real-time spectra. For a full grand-canonical Fock trace with imaginary-time evolution generated by K=H−μQK=H-\mu Q, bosonic and fermionic fields have the usual periodic and antiperiodic thermal boundary conditions. A fixed-charge projection needs additional care for fields that change charge.

Continue to Thermal and Nonequilibrium QFT for interacting thermal fields, screening, and finite-density methods. A static screening length and a real-time damping rate are different observables; neither can generally be read off from the other.

Use the Schwinger–Keldysh bridge when the question concerns a prepared state, a quench, or a causal expectation value. For unitary branch evolution and normalized ρ0\rho_0,

Z[J+,J−]=Tr⁡(UJ+ρ0UJ−†),Z[J,J]=1.Z[J_+,J_-]=\operatorname{Tr}(U_{J_+}\rho_0U_{J_-}^{\dagger}), \qquad Z[J,J]=1.

This construction retains the initial density operator while combining forward and backward evolution. The real-time chapters in Thermal and Nonequilibrium QFT extend it to self-energies, memory kernels, and controlled kinetic approximations. An imaginary-time equilibrium calculation alone does not specify an arbitrary quench.

Combine transport coefficients with hydrodynamic effective theory. Conservation supplies a balance equation; constitutive relations supply the current; equilibrium fluctuation relations fix the associated thermal noise.

The hydrodynamic chapters of Thermal and Nonequilibrium QFT add nonlinear fluctuations, relativistic causality, and systematic effective actions. Identify local equilibration and the slow fields before assuming ordinary diffusion: unscreened electric fields, momentum conservation, or integrability can change the mode structure.

Suppose you want the long-wavelength density response of a homogeneous normal system with screened interactions, finite compressibility, and sufficiently rapid momentum relaxation. In the classical thermal hydrodynamic regime, a single diffusive charge has

χnnR(q,ω)=χ Dq2Dq2−iω.\chi^R_{nn}(q,\omega)=\chi\,\frac{Dq^2}{Dq^2-i\omega}.

Here the source is H′=−∫ddx δμ nH\prime=-\int d^dx\,\delta\mu\,n, so the physical response uses the +i+i commutator convention with ℏ=1\hbar=1.

Thermodynamics determines χ=(∂n/∂μ)T\chi=(\partial n/\partial\mu)_T. A microscopic Kubo calculation or measurement determines DD. Hydrodynamics organizes their joint low-frequency response; a real-time fluctuation calculation also needs the current noise. The formula gives

lim⁡q→0lim⁡ω→0χnnR(q,ω)=χ,lim⁡ω→0lim⁡q→0χnnR(q,ω)=0.\lim_{q\to0}\lim_{\omega\to0}\chi^R_{nn}(q,\omega)=\chi, \qquad \lim_{\omega\to0}\lim_{q\to0}\chi^R_{nn}(q,\omega)=0.

The first experiment permits a nonuniform density to equilibrate before making its wavelength infinite. The second drives the exactly conserved uniform charge, which cannot respond dynamically in a closed system. A change of ensemble is a separate operation. This example explains why the state, source, and order of limits belong beside a field-theory formula.

For a calculation you are learning, keep its physical dimension, state, operator, source, cutoff, and limit order explicit. Return to the relevant derivation when one of these is unclear; more elaborate notation does not supply the missing assumption.

Choose a useful first route for each task: a critical order-parameter exponent; causal response after a quench; a conserved-density diffusion pole; a source-dependent effective action; fermionic propagators at finite density; matching a nonrelativistic contact interaction to scattering data.

Solution

Start respectively with RG and criticality; real-time Schwinger–Keldysh methods; hydrodynamics and transport; functional integrals and sources; thermal or finite-density fields; and nonrelativistic QFT with EFT matching. Finite-density methods also apply at zero temperature. The routes overlap: a microscopic transport calculation can need several of them, while a contact-scattering calculation need not introduce relativity.

Exercise 2: Diagnose an incomplete calculation

Section titled “Exercise 2: Diagnose an incomplete calculation”

A calculation writes Z=∫Dϕ e−S[ϕ]Z=\int\mathcal D\phi\,e^{-S[\phi]} and quotes a dc conductivity. Which missing information would let you decide whether that result follows?

Solution

First identify whether this is an equilibrium Euclidean integral, its fields and state, and its regulator. Then specify the source coupled to the physical current and the correlator produced by differentiation. If the calculation is Euclidean, explain the continuation to the retarded correlator, including any contact or diamagnetic terms. Finally state the thermodynamic, zero-wave-number, and zero-frequency limits and the approximation used. The partition-function notation alone supplies none of these response choices.