Physics 742 – Graduate Quantum Mechanics 2 Solutions to Chapter 18 5. [20] An electron is trapped in a 3D harmonic oscillator potential, H P 2 2m 12 m02 R 2 . It is in the ground state nx , ny , nz 0, 0, 0 . Photons are fired at the electron with frequency 0 , going in the z-direction, and polarized in the x-direction, ε xˆ . Calculate the differential cross section d d (summed over final polarizations, not integrated), and the total cross section . The amplitude for the scattering, according to the notes, Eq. (18.18) is FI e2 0V mI * ε rmI ε I rmI 2 2 F mI m The initial photon is polarized in the x-direction, and therefore the relevant matrix element will be m ax ax† 000 m 100 2m0 2m0 ε I rmI m X 000 The only relevant intermediate state, then, is the 100 state. We therefore have FI e2 0V 100, I * e2 m 2 2 ε F r100,I ε I r100,I V 2m 2 0 2 Fx* . 100, I 0 0 0 By Fermi’s Golden rule, the rate for this transition is then 2 2 2 e 2 2 2 2 FI EF EI Fx F . 2 2 0Vm 2 2 0 We wish to sum this over polarizations and final wave numbers of the photon. If we define as the angle between the final photon and the x-axis, then we would have 2 e 4 2 4 V m 2 0 2 2 2 2 2 2 0 Vcm 2 2 0 2 2 Fx F 2 kF , 2 2 4 c 2 2 2Vm 2 2 2 sin d F F dF F 0 2 0 d 3k F 2 2 2 2 2 4 Vcm 2 2 0 3 2 2 sin 2 F sin 2 d F . The rate is still inversely proportional to the volume. As usual, we convert this to a cross-section by dividing by the number density (which means multiplying by V) and dividing by the relative speed (c), so we have 2 2 4 c 2 m 2 02 2 2 sin 2 d F . The unintegrated version of this is the differential cross-section, or we can go ahead and integrate it for the total cross-section. 2 2 4 sin 2 8 2 2 4 d , and . 2 2 2 2 2 d c 2 m 2 2 2 2 3 c m 0 0 As expected, there is a huge enhancement near resonance, when 0 .