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QFT Bridge: S-Matrix

The scattering matrix maps asymptotic incoming states to asymptotic outgoing states. S-Matrix is the canonical nonrelativistic construction from Møller wave operators. This bridge asks what survives when the asymptotic states become multiparticle states of quantum fields.

The shared abstraction is

Sfi=⟨f,out∣i,in⟩.S_{fi} = \langle f,\mathrm{out}|i,\mathrm{in}\rangle.

The difference is what the states mean and how amplitudes are normalized.

In nonrelativistic scattering, one often starts from a free incoming state and constructs an outgoing-boundary scattering state:

∣ψ(+)⟩=∣ϕ⟩+G0(+)(E)V∣ψ(+)⟩.|\psi^{(+)}\rangle = |\phi\rangle + G_0^{(+)}(E)V|\psi^{(+)}\rangle.

The potential acts within a fixed-particle Hilbert space.

In QFT, the in and out states are Fock-space states. Particle number can change, so an SS-matrix element can describe processes such as

2→2,1→3,2→n.2\to2, \qquad 1\to3, \qquad 2\to n.

The fixed-particle potential picture is therefore only a special limiting intuition.

Nonrelativistic scattering often uses amplitudes f(θ,ϕ)f(\theta,\phi) defined by

ψ(r)∼eik⋅r+f(θ,ϕ)eikrr.\psi(\mathbf r) \sim e^{i\mathbf k\cdot\mathbf r} + f(\theta,\phi) \frac{e^{ikr}}{r}.

QFT usually defines an invariant amplitude M\mathcal M after factoring out momentum conservation:

⟨f∣S∣i⟩=⟨f∣i⟩+i(2π)4δ(4)(Pf−Pi)Mfi\langle f|S|i\rangle = \langle f|i\rangle + i(2\pi)^4\delta^{(4)}(P_f-P_i) \mathcal M_{fi}

in a common convention. Different texts move factors of ii, 2π2\pi, and normalization into different symbols.

The practical rule is simple: translate complete cross sections or rates, not isolated amplitudes.

In potential scattering, the Lippmann–Schwinger equation constructs scattering states from a Hamiltonian and boundary conditions. In QFT, the LSZ reduction formula extracts scattering amplitudes from time-ordered correlation functions by isolating external one-particle poles.

The analogy is:

asymptotic free states↔external particle poles.\text{asymptotic free states} \quad \leftrightarrow \quad \text{external particle poles}.

The implementation differs because QFT uses fields, relativistic normalization, and multiparticle phase space.

From Correlation Functions to QFT Observables explains why LSZ starts from a connected time-ordered correlator and what remains before it becomes a cross section.

The following ideas carry over directly:

  • amplitudes are complex and interfere;
  • unitarity constrains the SS-matrix;
  • resonances are tied to poles;
  • total probability is distributed among all allowed channels;
  • perturbation theory computes matrix elements order by order.

The following features change:

  • particle number is no longer fixed;
  • state normalization includes relativistic factors;
  • Lorentz-invariant phase space replaces simple solid-angle counting;
  • interactions come from field operators rather than a fixed potential;
  • spin, antiparticles, and crossing symmetry become structural.
  • Treating the nonrelativistic amplitude ff as if it were M\mathcal M.
  • Forgetting that QFT states live in Fock space.
  • Ignoring delta-function normalization when comparing SS-matrix elements.
  • Assuming LSZ is just the Lippmann–Schwinger equation in different notation.
  1. What is the shared meaning of SfiS_{fi} in QM and QFT?
Solution

In both settings, SfiS_{fi} is the amplitude for an incoming asymptotic state ii to be detected as an outgoing asymptotic state ff:

Sfi=⟨f,out∣i,in⟩.S_{fi} = \langle f,\mathrm{out}|i,\mathrm{in}\rangle.

The meaning and normalization of the states differ between nonrelativistic quantum mechanics and QFT.

  1. Why does particle production force a conceptual change from potential scattering to QFT scattering?
Solution

Potential scattering usually acts in a fixed-particle Hilbert space. QFT scattering acts on Fock space, where states with different particle numbers coexist. Processes such as 2→32\to3 or decays cannot be represented as ordinary one-particle scattering from a fixed potential without adding extra structure by hand.

  • J. R. Taylor, Scattering Theory: The Quantum Theory of Nonrelativistic Collisions, Dover, 2006.
  • M. E. Peskin and D. V. Schroeder, An Introduction to Quantum Field Theory, Addison-Wesley, 1995.
  • S. Weinberg, The Quantum Theory of Fields, Vol. I: Foundations, Cambridge University Press, 1995.
  • M. D. Schwartz, Quantum Field Theory and the Standard Model, Cambridge University Press, 2014.