Skip to content

Hydrogen Radial Wavefunctions

For ψnℓm=Rnℓ(r)Yℓm(θ,ϕ)\psi_{n\ell m}=R_{n\ell}(r)Y_\ell^m(\theta,\phi), define

aZ=4πϵ0ℏ2μZe2,ρ=2rnaZ.a_Z=\frac{4\pi\epsilon_0\hbar^2}{\mu Ze^2}, \qquad \rho=\frac{2r}{na_Z}.

The normalized bound-state radial function is

Rnℓ(r)=(2naZ)3(n−ℓ−1)!2n(n+ℓ)!e−ρ/2ρℓLn−ℓ−1(2ℓ+1)(ρ).R_{n\ell}(r) =\sqrt{\left(\frac{2}{na_Z}\right)^3 \frac{(n-\ell-1)!}{2n(n+\ell)!}} e^{-\rho/2}\rho^\ell L_{n-\ell-1}^{(2\ell+1)}(\rho).

Also,

unℓ=rRnℓ,Pnℓ(r)=r2∣Rnℓ(r)∣2=∣unℓ(r)∣2,u_{n\ell}=rR_{n\ell}, \qquad P_{n\ell}(r)=r^2|R_{n\ell}(r)|^2=|u_{n\ell}(r)|^2,

and the number of interior radial nodes is n−ℓ−1n-\ell-1.

⟨r⟩nℓ=aZ2[3n2−ℓ(ℓ+1)],\langle r\rangle_{n\ell} =\frac{a_Z}{2}[3n^2-\ell(\ell+1)], ⟨1r⟩n=1aZn2,⟨1r2⟩nℓ=1aZ2n3(ℓ+1/2).\left\langle\frac1r\right\rangle_n=\frac{1}{a_Zn^2}, \qquad \left\langle\frac1{r^2}\right\rangle_{n\ell} =\frac{1}{a_Z^2n^3(\ell+1/2)}.
  • ∫∣Yℓm∣2dΩ=1\int|Y_\ell^m|^2d\Omega=1 and ∫0∞r2∣Rnℓ∣2dr=1\int_0^\infty r^2|R_{n\ell}|^2dr=1.
  • n=1,2,…n=1,2,\ldots and 0≤ℓ≤n−10\le\ell\le n-1.
  • μ\mu is the electron–nucleus reduced mass; aZa_Z is not generally a0a_0.
SymbolMeaning
RnℓR_{n\ell}radial factor, dimensions L−3/2\mathsf L^{-3/2}
unℓu_{n\ell}reduced radial function, dimensions L−1/2\mathsf L^{-1/2}
PnℓP_{n\ell}radial shell density, dimensions L−1\mathsf L^{-1}
Lq(α)L_q^{(\alpha)}generalized Laguerre polynomial
aZa_Zreduced-mass, charge-ZZ Coulomb length
  • Do not normalize RR with drdr; its measure is r2drr^2dr.
  • The endpoint r=0r=0 is not counted as an interior radial node.
  • A radial function alone is not a complete orbital; attach YℓmY_\ell^m.
  • These are point-Coulomb bound states. Screening, relativistic structure, finite nuclear size, and continuum normalization require other treatments.

Derivation, low-lying examples, radial matrix elements, plots, exercises, and references are at Radial Wavefunctions.