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Quantum Dynamics and Formulations

Quantum dynamics studies how quantum states, observables, amplitudes, and probability distributions change with time. Its central object is the Hamiltonian-generated time evolution of a closed system.

In the Schrödinger picture,

iℏddt∣ψ(t)⟩=H(t)∣ψ(t)⟩,i\hbar\frac{d}{dt}\lvert\psi(t)\rangle =H(t)\lvert\psi(t)\rangle,

and the same evolution can be written using a time-evolution operator:

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

This volume explains the many equivalent languages built around that idea. For the local orientation chapter, start with Overview and Map of Quantum Dynamics, then use Foundations of Time Evolution, Pictures of Quantum Mechanics, and Operator Dynamics for the common equations behind the later formulations.

No single representation makes every problem simple. The Schrödinger picture is natural for wavefunctions and numerical state propagation. The Heisenberg picture is natural for operator motion, symmetries, and constants of motion. The interaction picture isolates perturbations. Propagators compute transition amplitudes. Green functions expose spectra and boundary conditions. Path integrals connect amplitudes to the action. Phase-space methods clarify the classical limit.

The formulations are not competing theories. They are different coordinate systems on the same quantum mechanics.

NeedUseful formulationFirst page
Track a state in timeSchrödinger pictureSchrödinger Picture
Track observables in timeHeisenberg pictureHeisenberg Picture
Separate solvable and perturbing dynamicsInteraction pictureInteraction Picture
Evolve observables, density operators, and operator algebrasOperator dynamicsOperator Dynamics
Compute transition amplitudesPropagators and kernelsPropagators and Kernels
Analyze spectra and boundary conditionsGreen functions and resolventsGreen Functions and Resolvents
Connect to action principlesPath integralsPath Integral Formulation
Study the classical limitPhase-space and semiclassical methodsPhase-Space Formulation
Validate numerical evolutionReproducible notebooksNotebooks and Worked Examples
Prepare for field theoryTime ordering, propagators, path integralsWhy Dynamics Matters for QFT

Some linked pages are launch targets for this volume and may appear after the overview pages.

This volume owns closed-system time evolution and equivalent formulations. It does not replace:

  • Core Formalism for states, observables, Born rule, and postulates;
  • Wave Mechanics and Model Systems for solving standard one-particle Hamiltonians;
  • future approximation and scattering pages for Fermi golden rule, WKB, and detailed scattering applications;
  • future open-system pages for Lindblad dynamics, decoherence, and quantum trajectories.

For a first dynamics pass, read Foundations of Time Evolution, then Pictures of Quantum Mechanics through Schrödinger picture, Heisenberg picture, and Ehrenfest theorem.

For a graduate formalism pass, add operator dynamics, interaction picture, time ordering, Dyson expansion, propagators, Green functions, and path integrals.

For a computational pass, use Notebooks and Worked Examples to pair analytic benchmarks with Fourier grids, propagators, product formulas, imaginary-time projection, Wigner transforms, and Floquet spectra.

For a field-theory bridge, focus on Heisenberg picture, interaction picture, time ordering, propagators, Green functions, path integrals, and correlation functions.

  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  • L. S. Schulman, Techniques and Applications of Path Integration, Wiley, 1981.
  • M. E. Peskin and D. V. Schroeder, An Introduction to Quantum Field Theory, Addison-Wesley, 1995.
  1. Name two formulations that give the same expectation values but move the time dependence to different objects.
Solution

The Schrödinger and Heisenberg pictures are the standard pair. In the Schrödinger picture, states carry the main time dependence. In the Heisenberg picture, states are fixed and observables carry the time dependence. Expectation values agree when the pictures are transformed consistently.