“Know how to solve every problem that has been solved.” “What I cannot create, I do not understand.” — Richard Feynman

What orbital energies mean

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Lesson 19 of 24 standard ~5 min

The SCF hands you a ladder of orbital energies ε. They are not slices of the total energy (summing them double-counts repulsion) — so what physical thing are they? Koopmans' theorem supplies the answer: yank an electron out of orbital i, freeze every other orbital in place, and the energy you pay is exactly −εᵢ. For the loosest electron:

standardMultiple choice

According to Koopmans' theorem, the ionization potential of a molecule is approximately…

Go deeper ↓Hartree-Fock Method

The frozen-orbital assumption is obviously false — the cation relaxes — and Hartree-Fock is missing correlation on top. Yet Koopmans IPs land within a volt or so of experiment surprisingly often, and the reason is an error cancellation: relaxation (ignored) would lower the ion, so freezing overestimates the IP; correlation (ignored) stabilizes the electron-rich neutral more, so neglecting it underestimates the IP. Two wrongs, opposite signs.

hardMultiple choice

Koopmans' theorem makes two crude approximations, yet its ionization potentials are often surprisingly decent. Why?

Go deeper ↓Hartree-Fock Method

This is also the cleanest example of a habit worth building: every quantity the calculation prints should be answerable to an experiment. Orbital energies answer to photoelectron spectroscopy — that is why the HOMO's ε matters and the absolute zero of the ladder doesn't.