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From Propagators in QM to Propagators in QFT

The word “propagator” means different but related things in quantum mechanics and quantum field theory. In nonrelativistic quantum mechanics, the basic propagator is a kernel of the time-evolution operator:

K(xf,tf;xi,ti)=⟨xf∣U(tf,ti)∣xi⟩.K(x_f,t_f;x_i,t_i) = \langle x_f|U(t_f,t_i)|x_i\rangle.

In QFT, the most common propagator is a time-ordered two-point function of fields:

ΔF(x−y)=⟨0∣T{ϕ(x)ϕ(y)}∣0⟩.\Delta_F(x-y) = \langle 0| \mathcal T\{\phi(x)\phi(y)\} |0\rangle.

Both objects describe how disturbances, amplitudes, or correlations connect spacetime points, but they are not the same kind of mathematical object. This page is a translation guide.

For a single nonrelativistic particle, the coordinate-space propagator kernel is

K(xf,tf;xi,ti)=⟨xf∣U(tf,ti)∣xi⟩.K(x_f,t_f;x_i,t_i) = \langle x_f|U(t_f,t_i)|x_i\rangle.

It evolves wavefunctions:

ψ(xf,tf)=∫dxi K(xf,tf;xi,ti)ψ(xi,ti).\psi(x_f,t_f) = \int dx_i\, K(x_f,t_f;x_i,t_i)\psi(x_i,t_i).

For a time-independent Hamiltonian with energy eigenfunctions ψn(x)\psi_n(x),

K(xf,t;xi,0)=∑nψn(xf)ψn∗(xi)e−iEnt/ℏ,K(x_f,t;x_i,0) = \sum_n \psi_n(x_f)\psi_n^*(x_i) e^{-iE_nt/\hbar},

with continuum contributions added when the spectrum is not purely discrete.

This object is an amplitude kernel. It is not itself a probability:

∣K(xf,tf;xi,ti)∣2|K(x_f,t_f;x_i,t_i)|^2

is not generally a normalized transition probability density unless a specific preparation and measurement protocol has been specified.

The canonical quantum-mechanics page is Propagator Kernel.

Quantum mechanics also uses Green functions as inverse kernels. For a time-independent Hamiltonian,

G(z)=(z−H)−1G(z) = (z-H)^{-1}

is the resolvent. Its position-space kernel is

G(x,x′;z)=⟨x∣(z−H)−1∣x′⟩.G(x,x';z) = \langle x|(z-H)^{-1}|x'\rangle.

Boundary values such as

G±(E)=lim⁡ϵ→0+1E−H±iϵG^\pm(E) = \lim_{\epsilon\to0^+} \frac{1}{E-H\pm i\epsilon}

select incoming or outgoing scattering prescriptions. Time-domain retarded, advanced, and time-ordered Green functions answer different response or ordering questions.

Thus even inside ordinary quantum mechanics, “propagator” can mean at least two related objects:

ObjectTypical formulaMain role
Time-evolution kernel$\langle x_fU(t_f,t_i)
Energy Green function$\langle x(E-H\pm i0)^{-1}

The distinction is developed in What Is a Green Function?.

In relativistic scalar QFT, a standard Feynman propagator is the vacuum time-ordered two-point function

ΔF(x−y)=⟨0∣T{ϕ(x)ϕ(y)}∣0⟩.\Delta_F(x-y) = \langle0| \mathcal T\{\phi(x)\phi(y)\} |0\rangle.

For a free real scalar field, a common convention writes

ΔF(x−y)=∫d4p(2π)4i e−ip⋅(x−y)p2−m2+i0,\Delta_F(x-y) = \int\frac{d^4p}{(2\pi)^4} \frac{i\,e^{-ip\cdot(x-y)}} {p^2-m^2+i0},

using the mostly-minus convention

p2=(p0)2−p2.p^2=(p^0)^2-\mathbf p^2.

Some texts absorb factors of ii into the definition of ΔF\Delta_F or define iΔFi\Delta_F as the propagator. The convention must be checked before comparing Feynman rules.

The conceptual shift is the important part: the QFT propagator is not the matrix element of a one-particle position-basis time-evolution operator. It is a field correlation function in a specified state, usually the vacuum. It becomes a particle-propagation object only after additional interpretation, such as free-field mode expansion or scattering theory with asymptotic particle states.

Time Ordering and the Feynman Prescription

Section titled “Time Ordering and the Feynman Prescription”

The time-ordering symbol means

T{ϕ(x)ϕ(y)}={ϕ(x)ϕ(y),x0>y0,ϕ(y)ϕ(x),y0>x0,\mathcal T\{\phi(x)\phi(y)\} = \begin{cases} \phi(x)\phi(y), & x^0\gt y^0,\\ \phi(y)\phi(x), & y^0\gt x^0, \end{cases}

for bosonic fields, ignoring equal-time distribution subtleties. The Feynman i0i0 prescription in momentum space selects how the poles are bypassed:

1p2−m2+i0.\frac{1}{p^2-m^2+i0}.

This prescription is the analytic imprint of time ordering and vacuum boundary conditions. It is not interchangeable with the retarded prescription. A retarded propagator instead vanishes outside the future response region:

GR(x−y)=0for x0<y0.G_R(x-y)=0 \qquad \text{for }x^0\lt y^0.

Feynman propagators are central in perturbative scattering amplitudes. Retarded propagators are central in causal response. Euclidean propagators are central in imaginary-time and statistical formulations. They are related by analytic continuation under appropriate assumptions, but they answer different questions.

From Euclidean Time to Euclidean QFT develops the thermal-circle and Matsubara structure of the Euclidean case.

Relativistic QFT imposes locality conditions that have no direct analogue in single-particle nonrelativistic quantum mechanics. Causality, Support, and Interpretation in Nonrelativistic QM compares the Schrödinger kernel, commutator distribution, retarded response, Feynman propagator, and Wightman function in detail. For a bosonic scalar field, microcausality states

[ϕ(x),ϕ(y)]=0when (x−y)2<0.[\phi(x),\phi(y)]=0 \qquad \text{when }(x-y)^2\lt0.

This says spacelike separated field measurements are compatible. It does not mean the Feynman propagator itself vanishes at spacelike separation. The Feynman propagator is a time-ordered correlation function, not the commutator that directly measures causal influence.

The retarded commutator-type response is the object tied most directly to causal propagation:

GR(x−y)=θ(x0−y0)⟨0∣[ϕ(x),ϕ(y)]∣0⟩G_R(x-y) = \theta(x^0-y^0) \langle0|[\phi(x),\phi(y)]|0\rangle

up to conventional factors. The commutator vanishes at spacelike separation in a local relativistic theory.

In a free scalar theory, the propagator has a pole at

p2=m2,p^2=m^2,

which matches the relativistic mass shell for a particle of mass mm. In interacting theories, the full two-point function has a richer spectral structure. A schematic Källén–Lehmann representation is

ΔF(p)=∫0∞dμ2 iρ(μ2)p2−μ2+i0.\Delta_F(p) = \int_0^\infty d\mu^2\, \frac{i\rho(\mu^2)} {p^2-\mu^2+i0}.

An isolated pole can represent a stable particle; branch cuts represent multiparticle continua; resonances appear through analytic continuation. A field need not create a single particle cleanly, and a particle need not correspond to a unique elementary field.

Therefore the safest statement is:

QFT propagators encode field correlations and spectral data.\text{QFT propagators encode field correlations and spectral data.}

Particle language is often correct and extremely useful in scattering regimes, but it is not the definition.

Quantum-mechanical objectQFT analogueWarning
K(xf,tf;xi,ti)K(x_f,t_f;x_i,t_i)transition kernels or path-integral amplitudesQFT usually uses field configurations, not one particle coordinate
(E−H±i0)−1(E-H\pm i0)^{-1}momentum-space denominators and spectral Green functionsi0i0 prescriptions encode boundary conditions
time-ordered correlatorFeynman propagatorconvention-dependent factors of ii
retarded responseretarded field Green functioncausal response differs from Feynman ordering
spectral polesparticle masses or bound-state energiesinteracting spectra also have cuts and resonances
source responsegenerating functional derivativesfields, sources, and normalization conventions must be fixed
  • Treating a QFT Feynman propagator as a literal probability amplitude for a classical particle path.
  • Forgetting that KK, GRG_R, GFG_F, Euclidean correlators, and resolvents are different objects.
  • Dropping the i0i0 prescription as if it were optional notation.
  • Assuming the Feynman propagator must vanish outside the light cone.
  • Comparing QFT and many-body propagator conventions without checking factors of ii, signs, and Fourier transforms.
  • Ignoring the state: vacuum, thermal, in-in, and scattering correlators are not the same.
  • M. E. Peskin and D. V. Schroeder, An Introduction to Quantum Field Theory, Addison-Wesley, 1995.
  • M. D. Schwartz, Quantum Field Theory and the Standard Model, Cambridge University Press, 2014.
  • S. Weinberg, The Quantum Theory of Fields, Volume I: Foundations, Cambridge University Press, 1995.
  • A. Zee, Quantum Field Theory in a Nutshell, 2nd ed., Princeton University Press, 2010.
  • A. L. Fetter and J. D. Walecka, Quantum Theory of Many-Particle Systems, Dover, 2003.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  1. Show how the quantum-mechanical propagator kernel evolves a wavefunction.
Solution

Start from

∣ψ(tf)⟩=U(tf,ti)∣ψ(ti)⟩.\lvert\psi(t_f)\rangle = U(t_f,t_i)\lvert\psi(t_i)\rangle.

Insert a position resolution of identity at the initial time:

I=∫dxi ∣xi⟩⟨xi∣.I=\int dx_i\,|x_i\rangle\langle x_i|.

Taking the final position amplitude gives

ψ(xf,tf)=∫dxi ⟨xf∣U(tf,ti)∣xi⟩ψ(xi,ti).\psi(x_f,t_f) = \int dx_i\, \langle x_f|U(t_f,t_i)|x_i\rangle \psi(x_i,t_i).

Thus

K(xf,tf;xi,ti)=⟨xf∣U(tf,ti)∣xi⟩K(x_f,t_f;x_i,t_i) = \langle x_f|U(t_f,t_i)|x_i\rangle

is the evolution kernel.

  1. Why is a QFT Feynman propagator not simply a one-particle wavefunction kernel?
Solution

The Feynman propagator is a vacuum expectation value of time-ordered field operators:

ΔF(x−y)=⟨0∣T{ϕ(x)ϕ(y)}∣0⟩.\Delta_F(x-y) = \langle0|\mathcal T\{\phi(x)\phi(y)\}|0\rangle.

It is a correlation function of fields in a specified state. A one-particle kernel instead evolves a wavefunction between position eigenstates. In free or scattering regimes the field correlator has a particle interpretation, but that interpretation is additional structure, not the definition.

  1. Which object is more directly tied to causal response: the Feynman propagator or the retarded propagator?
Solution

The retarded propagator is more directly tied to causal response because it vanishes before the source acts:

GR(x−y)=0for x0<y0.G_R(x-y)=0 \qquad \text{for }x^0\lt y^0.

The Feynman propagator is time ordered and is used in perturbative amplitudes. It is not the same as the causal response function.

  1. What does the i0i0 prescription do in a propagator denominator?
Solution

The i0i0 prescription specifies how singularities are approached in the complex energy or momentum plane. In

1p2−m2+i0,\frac{1}{p^2-m^2+i0},

it tells how the poles are displaced and encodes the Feynman time-ordering boundary condition. Different prescriptions give different Green functions, such as retarded or advanced ones.

  1. What spectral information is suggested by a pole at p2=m2p^2=m^2?
Solution

For a free scalar field, a pole at

p2=m2p^2=m^2

matches the relativistic mass shell of a particle with mass mm. In an interacting theory, an isolated pole can indicate a stable particle state, while cuts and more complicated analytic structures represent multiparticle continua or resonances.