Zeeman effect — where it appears
Named by 3 essays across 3 fields — each of them below, with the objects they name alongside it.
Complex harmonics against real ones
The p orbitals every chemist draws are not eigenfunctions of anything. They are real combinations of the complex solutions, chosen because they point along axes — and the choice is invisible until a magnetic field makes it matter.
The g-value is the orbital coming back
A ligand field quenches the orbital angular momentum of a d electron, and spin-orbit coupling gives some of it back — upward for a shell more than half full and downward for one less than half full. Which way a resonance line moves counts the electrons, and the size of the move comes from two matrix elements and one optical splitting.
How nearly a broken symmetry survives
The hydrogen shell's extra symmetry is what makes its Stark effect linear, and a real atom does not have it. Screening splits the shell, and the field needed to overcome the splitting and restore the linear behaviour is a curve — from forty thousand volts a centimetre at a quantum defect of 0.0004 to thirty million at a defect of 0.21.
Named alongside it
The objects these essays reach for when they reach for this one.
DegeneracyAngular momentumMatrix elementQuantum numbersBasisClosed formConserved quantityConventionCovalent bondingd orbitalsEffective nuclear chargeExpectation value