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Normalization Examples

Normalization fixes the scale of probabilities. Before using any example, identify whether the object is a square-integrable state, a generalized eigenstate, a radial function, a spinor, a density matrix, or a scattering state.

For a normalizable wavefunction in one dimension,

∫−∞∞∣ψ(x)∣2 dx=1.\int_{-\infty}^{\infty}\lvert\psi(x)\rvert^2\,dx=1.

For a state vector,

⟨ψ∣ψ⟩=1.\langle\psi\rvert\psi\rangle=1.

For a density matrix,

Tr⁡ρ=1,ρ≥0.\operatorname{Tr}\rho=1, \qquad \rho\ge 0.

The compact formula card is Normalization. The wave-mechanics teaching page is Normalization Conventions.

Example TypeLearnWhat to Watch
One-dimensional wavefunctionExercise Sets, Set 1Integration limits and units
Coordinate-space probabilityWavefunctions and Probability DensityDensity versus probability
Position-space inner productCoordinate RepresentationCompleteness convention
Radial wavefunctionRadial Schrödinger EquationR(r)R(r) versus u(r)=rR(r)u(r)=rR(r)
SpinorSpin-Half Hilbert SpaceBasis order and phase
Density matrixDensity OperatorsTrace one and positivity
Scattering stateReflection and Transmission CoefficientsFlux normalization rather than square integrability
  • Treating ∣ψ(x)∣2\lvert\psi(x)\rvert^2 as a probability without integrating over a region.
  • Forgetting the spherical measure r2dr dΩr^2dr\,d\Omega.
  • Normalizing R(r)R(r) as if it were u(r)u(r).
  • Applying square-integrable normalization to plane waves without stating a box, delta, or wave-packet convention.
  • Checking Tr⁡ρ=1\operatorname{Tr}\rho=1 but not positivity for a mixed state.

For ψ(x)=Ae−κ∣x∣\psi(x)=Ae^{-\kappa\lvert x\rvert} with κ>0\kappa>0,

1=∫−∞∞A2e−2κ∣x∣ dx=2A2∫0∞e−2κx dx=A2κ.1=\int_{-\infty}^{\infty}A^2e^{-2\kappa\lvert x\rvert}\,dx =2A^2\int_0^\infty e^{-2\kappa x}\,dx =\frac{A^2}{\kappa}.

Thus A=κA=\sqrt{\kappa} if AA is chosen real and positive. The dimension check is useful: AA has units of L−1/2L^{-1/2} in one dimension.

  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • C. Cohen-Tannoudji, B. Diu, and F. Laloe, Quantum Mechanics, Wiley, 1977.
  1. A radial solution is written as ψ(r,θ,ϕ)=R(r)Yℓm(θ,ϕ)\psi(r,\theta,\phi)=R(r)Y_{\ell m}(\theta,\phi), with normalized spherical harmonic. Which integral normalizes RR?
Solution

Use ∫0∞∣R(r)∣2r2 dr=1\int_0^\infty \lvert R(r)\rvert^2r^2\,dr=1. If u(r)=rR(r)u(r)=rR(r) is used instead, the condition becomes ∫0∞∣u(r)∣2 dr=1\int_0^\infty\lvert u(r)\rvert^2\,dr=1.