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Which Formulation Should I Use?

The best formulation is the one that makes the question simple while keeping the assumptions visible. None is universally superior.

TaskStart withWhy
Find the state at time ttSchrödinger pictureIt evolves ∣ψ(t)⟩\lvert\psi(t)\rangle directly
Show a probability is conservedUnitary evolutionNorm preservation is explicit
Track an observable such as x(t)x(t) or Sz(t)S_z(t)Heisenberg pictureOperators obey equations of motion
Treat a weak time-dependent perturbationInteraction pictureThe solvable part is factored out
Compute amplitude from one position to anotherPropagator kernelIt gives the coordinate-space transition amplitude
Extract spectral informationResolvent or Green functionPoles and branch cuts encode spectra
Use the action and stationary phasePath integralHistories are weighted by eiS/ℏe^{iS/\hbar}
Compare with classical phase spaceWigner-Moyal formulationIt represents states and observables on phase space
Study a periodic driveFloquet formulationOne-period evolution becomes central
Prepare for field theoryInteraction picture, Green functions, path integralsThese become standard field-theory tools

Use the Schrödinger picture or an explicit time-evolution operator:

∣ψ(t)⟩=U(t,t0)∣ψ(t0)⟩.\lvert\psi(t)\rangle =U(t,t_0)\lvert\psi(t_0)\rangle.

For wave mechanics, propagators and numerical methods can also be useful, but the conceptual home is state evolution.

If the operator has simple dynamics, use the Heisenberg picture:

dAHdt=iℏ[H,AH]+(∂A∂t)H.\frac{dA_H}{dt} =\frac{i}{\hbar}[H,A_H] +\left(\frac{\partial A}{\partial t}\right)_H.

This is especially efficient for oscillator ladder operators, spin precession, constants of motion, and symmetry arguments.

I Have a Small Perturbation Switched On in Time

Section titled “I Have a Small Perturbation Switched On in Time”

Use the interaction picture. Write

H(t)=H0+V(t),H(t)=H_0+V(t),

solve the H0H_0 motion exactly, and let the interaction-picture state evolve with the transformed perturbation. Detailed transition-rate calculations belong in approximation and scattering pages, but the formal language begins here.

Use a propagator:

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

The propagator is an amplitude, not a probability. Probabilities require taking appropriate absolute squares or integrating against wavefunctions.

Use the resolvent or a Green function. The resolvent

G(z)=(z−H)−1G(z)=(z-H)^{-1}

packages spectral information and becomes especially important in scattering, response theory, and many-body physics.

Use more than one tool. Ehrenfest theorem gives equations for expectation values, stationary phase explains why classical paths dominate certain limits, and the Phase-Space Formulation explains how Wigner functions place quantum states on phase space without turning them into ordinary probability distributions.

  • Do not use e−iH(t−t0)/ℏe^{-iH(t-t_0)/\hbar} for a time-dependent Hamiltonian unless the relevant Hamiltonians commute at different times or the expression has been justified.
  • Do not treat a propagator as a probability.
  • Do not use path integrals to bypass operator-ordering questions.
  • Do not assume the Heisenberg picture is only philosophical; it is often the most efficient calculational language.
  • Do not use the interaction picture as a synonym for perturbation theory. It is an exact rewriting before approximations are made.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • C. Cohen-Tannoudji, B. Diu, and F. Laloë, Quantum Mechanics, Wiley, 1977.
  1. A Hamiltonian is H(t)=H0+V(t)H(t)=H_0+V(t), where H0H_0 is exactly solvable and V(t)V(t) is weak. Which formulation should you try first?
Solution

The interaction picture is the natural first choice. It factors out the exactly solvable H0H_0 evolution and leaves the transformed perturbation to drive the remaining dynamics.