Separation of variables in the central Coulomb potential gives . The radial wavefunction depends on and , independently of . For the hydrogen radial wavefunction in the first excited shell, put . The Bohr radius is , where is the electron–proton reduced mass. Choose the real phases
Near the origin, , whereas . More generally, regular hydrogen radial wavefunctions behave as . At large , both displayed functions have a polynomial factor proportional to multiplying ; approaches zero from below and from above with these phase choices.
The radial wavefunction crosses zero once, at , and has its negative minimum at . The radial wavefunction has no radial node at positive , and reaches its maximum at . The count is ; neither the origin nor the limit at infinity is counted as a radial node. These are sketches of , rather than of or the radial probability density .
Figure 1.
Hydrogen radial wavefunctions in the first excited shell
. The horizontal coordinate is measured in Bohr radii; the vertical coordinate is the radial wavefunction multiplied by the Bohr radius to the power three halves. Details.
Both and commute with and are odd under parity. Their angular selection rules therefore require the same magnetic quantum number and opposite orbital parity. Within the nonrelativistic point-Coulomb hydrogen atom eigenspace, the only angularly permitted off-diagonal pair is and .
Those necessary angular conditions do not guarantee a nonzero matrix element. For the Coulomb potential Hamiltonian ,
All states within this exact eigenspace have the same energy, so every projected matrix element vanishes. In contrast, the position matrix element is nonzero: with conventional real spherical harmonics and hydrogen radial wavefunction in the first excited shell, . Its sign depends on basis phases, while its magnitude does not.
Thus the electric-dipole selection rules for hydrogen allow a linear position perturbation to mix these degenerate states, but a momentum perturbation cannot be assigned the same matrix merely from parity. The conclusion concerns the unperturbed Coulomb eigenspace; degeneracy-breaking interactions require their own energy eigenstates and matrix elements.