Scattering Theory
12.1 Partial Wave Analysis
Section titled “12.1 Partial Wave Analysis”For a spherically symmetric potential The scattering amplitude can be expanded in partial waves:
Where is the phase shift for partial wave .
Optical theorem:
Partial wave unitarity bound: So the maximum contribution of partial wave to the cross section is:
12.2 The Born Approximation
Section titled “12.2 The Born Approximation”For a weak potential, the scattering amplitude to first order is:
Where is the scattered wave vector and is the momentum transfer.
For the Yukawa potential :
Setting (Coulomb potential), this reproduces the Rutherford scattering formula.
12.3 Resonance Scattering
Section titled “12.3 Resonance Scattering”When the scattering energy is near a quasi-bound state, the phase shift passes through (resonance):
Where is the resonance energy and is the width. The cross section has the Breit—Wigner form:
At resonance (): (unitarity limit).
Worked Example 12.1: Low-Energy Scattering and Scattering Length
For -wave scattering () at low energy (), only the phase shift contributes:
Where the scattering length is defined by as .
For a hard sphere of radius : (exact), giving and (four times the geometric cross section --- a purely quantum result).
For the He—He system: nm (positive, indicating a repulsive effective potential). For the neutron—proton system (triplet): fm (positive, with a bound state --- the deuteron). For singlet: fm (negative, indicating a virtual state).
Worked Example 12.2: Born Approximation for a Gaussian Potential
Consider .
The total cross section:
At low energy (): (independent of ), giving:
The Born approximation is valid when I.e., the potential is weak compared to the kinetic energy associated with the length scale .
Common Pitfalls (Additional)
Section titled “Common Pitfalls (Additional)”Symmetrisation applies to the full wavefunction: For fermions, the overall wavefunction (spatial spin any other degrees of freedom) must be antisymmetric. A symmetric spatial part requires an antisymmetric spin part (singlet), and vice versa. Do not apply (anti)symmetrisation to spatial and spin parts separately without ensuring the correct combined symmetry.
The variational principle gives an upper bound: always. If you obtain a variational energy lower than the known exact ground state energy, you have made an error in the calculation (wrong normalisation, incorrect matrix element, or the trial function is not in the correct Hilbert space).
Fermi’s Golden Rule applies to transitions to a continuum: For transitions to discrete states, use the Rabi formula instead. The density of states is essential --- if it is zero, the transition rate is zero regardless of the matrix element.
The Born approximation assumes a weak potential: The condition is where is the range of the potential. For strong potentials (like the nuclear potential or hard spheres), the Born approximation gives qualitatively wrong results. Use partial wave analysis instead.
Resonances require careful treatment: Near a resonance, perturbation theory breaks down. The Breit—Wigner formula is non-perturbative in the width . The scattering length can be much larger than the range of the potential near a resonance (the unitarity limit).
Problems (Additional)
Section titled “Problems (Additional)”Problem 19: Exchange Energy in Lithium
Lithium () has the electron configuration . Using the variational method with for the electrons:
(a) Calculate for the electrons, treating the electron as a perturbation.
(b) Calculate the ionisation energy (removing the electron) and compare with the experimental value of 5.39 eV.
(c) Explain why the electron is effectively screened by .
Solution:
(a) For the electrons, the effective charge is reduced from by screening from the other electron and partial penetration of the electron. The electrons screen each other partially: using the helium result, .
(b) The electron sees an effective nuclear charge of (Slater’s rules). The energy:
E_{2s} = -\frac{Z_{\text{eff}^2}{n^2}\times 13.6\ \text{eV} = -\frac{1.3^2}{4}\times 13.6 = -\frac{1.69}{4}\times 13.6 = -5.75\ \text{eV}}
The ionisation energy is eV, close to the experimental 5.39 eV. The discrepancy reflects the crudeness of the Slater screening constants.
(c) The electron has significant radial extent beyond the core, so it sees a nearly bare nuclear charge at small but is screened by both electrons at large . The effective charge (using Hartree—Fock) represents this average screening.
Problem 20: Partial Wave Analysis for Square Well
Consider scattering from the attractive square well for and for .
(a) Show that the -wave phase shift satisfies:
Where and .
(b) Show that a bound state exists at energy when where .
(c) Show that the scattering length diverges as a new bound state appears.
Solution:
(a) Inside the well (), the radial wavefunction for is . Outside (), .
Matching and at :
Wait: .
(b) A bound state has So where . The bound state condition is that the exterior solution decays exponentially: . Matching:
As : So Giving (the threshold for the first bound state).
(c) The scattering length . As , So:
As : (diverges), changing sign as the bound state appears.