Advanced Quantum Mechanics · Tutorial 2c

Spectrum and revivals of the quantum pendulum

The Josephson Hamiltonian H = p²/2m − λ cos q, solved exactly and compared with the semiclassical picture. The first tab places Bohr–Sommerfeld orbits next to the exact eigenstates; the second follows a coherent state through collapse and revival, long after the classical description has failed.

levels below E = λ: — 16√(mλ)/h = — oscillation

Phase space

oscillating rotatingshading: Husimi

Level spacing

exact ħωcl(E)

Selected eigenstate

— exact |ψj|² WKB / classical density

Orbits. Each coloured curve is a classical orbit picked by Bohr–Sommerfeld: area (n + ½)h inside the separatrix, and nh under a rotating orbit, which has no turning points. Rotating orbits come in pairs, one for each direction, at the same energy.

Spacing. Dots are exact gaps Ej+1 − Ej. Below the separatrix they follow ħωcl(E) and dip where the period diverges. Above it they split into near-zero gaps inside a pair and gaps of ħωcl between pairs.

Eigenstate. The exact density oscillates around the WKB density 2/(Tcl v(q)), the fraction of time the classical particle spends at q. Its Husimi function sits on the quantized orbit.