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Time-Independent Hamiltonians

A Hamiltonian is time independent when it has no explicit dependence on the time parameter. In that case the time-evolution operator is the ordinary exponential

U(t,t0)=e−iH(t−t0)/ℏ.U(t,t_0)=e^{-iH(t-t_0)/\hbar}.

This is the simplest and most important exact solution of closed-system quantum dynamics.

The formula applies when the same Hamiltonian HH generates evolution throughout the interval from t0t_0 to tt. It does not require HH to be diagonal in the basis being used, but it does require HH not to change with time.

For unbounded Hamiltonians, the exponential is defined through spectral theory. In finite dimensions, it is the usual matrix exponential.

If HH has a discrete spectral decomposition

H=∑nEnPn,H=\sum_n E_n P_n,

then

U(t,t0)=∑ne−iEn(t−t0)/ℏPn.U(t,t_0) =\sum_n e^{-iE_n(t-t_0)/\hbar}P_n.

For nondegenerate eigenstates, Pn=∣En⟩⟨En∣P_n=\lvert E_n\rangle\langle E_n\rvert, so

U(t,t0)=∑ne−iEn(t−t0)/ℏ∣En⟩⟨En∣.U(t,t_0) =\sum_n e^{-iE_n(t-t_0)/\hbar} \lvert E_n\rangle\langle E_n\rvert.

This makes energy-basis evolution especially transparent: each energy component acquires a phase.

If an energy level is degenerate, every state inside that eigenspace gets the same phase under HH alone. Dynamics inside the degenerate subspace becomes nontrivial only if another term is added, a different observable is measured, or the basis choice matters for interpretation.

For continuous spectra, sums are replaced by spectral integrals. The free particle is the standard example: momentum components evolve by phases determined by E=p2/(2m)E=p^2/(2m).

The formal lesson is unchanged. Diagonalize the Hamiltonian, attach phases to spectral components, then transform back if needed.

In a finite-dimensional basis, HH is a Hermitian matrix. If it is diagonalized as

H=VDV†,H=V D V^\dagger,

then

e−iHτ/ℏ=Ve−iDτ/ℏV†,τ=t−t0.e^{-iH\tau/\hbar} = V e^{-iD\tau/\hbar}V^\dagger, \qquad \tau=t-t_0.

This is often the stable way to compute exact finite-dimensional time evolution.

For a diagonal two-level Hamiltonian

H=ℏω2σz,H=\frac{\hbar\omega}{2}\sigma_z,

the evolution is

U(t,0)=(e−iωt/200eiωt/2).U(t,0) = \begin{pmatrix} e^{-i\omega t/2} & 0\\ 0 & e^{i\omega t/2} \end{pmatrix}.

For the harmonic oscillator,

H=ℏω(a†a+12),H=\hbar\omega\left(a^\dagger a+\frac12\right),

number states evolve as

∣n;t⟩=e−iω(n+1/2)t∣n⟩.\lvert n;t\rangle =e^{-i\omega(n+1/2)t}\lvert n\rangle.
  • Using the exponential formula for a time-dependent Hamiltonian without checking commutators.
  • Thinking a time-independent Hamiltonian means all observables are time independent.
  • Forgetting relative phases between different energy eigenstates.
  • Treating degeneracy as if it automatically fixes a preferred basis inside the degenerate subspace.
  • Ignoring domain issues for unbounded Hamiltonians in rigorous arguments.
  • 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.
  • M. Reed and B. Simon, Methods of Modern Mathematical Physics I: Functional Analysis, revised and enlarged ed., Academic Press, 1980.
  1. Suppose H=∑nEnPnH=\sum_n E_nP_n. Show that U(t,t0)=∑ne−iEn(t−t0)/ℏPnU(t,t_0)=\sum_n e^{-iE_n(t-t_0)/\hbar}P_n satisfies the operator Schrödinger equation.
Solution

Differentiate the spectral expression:

iℏ∂U∂t=∑nEne−iEn(t−t0)/ℏPn.i\hbar\frac{\partial U}{\partial t} = \sum_n E_n e^{-iE_n(t-t_0)/\hbar}P_n.

Since HPn=EnPnHP_n=E_nP_n, the right-hand side is HU(t,t0)HU(t,t_0).