Partial wave unitarity bound:sin2δl≤1So the maximum contribution of partial wave l to the cross section is:
σlmax=k24π(2l+1)
12.2 The Born Approximation
For a weak potential, the scattering amplitude to first order is:
f(θ,ϕ)≈−2πℏ2m∫e−ik"⋅r′V(r′)d3r′
Where k′ is the scattered wave vector and q=k′−k is the momentum transfer.
For the Yukawa potential V(r)=(V0/r)e−μr:
f(θ)=−ℏ2(μ2+q2)2mV0,q=2ksin(θ/2)
Setting μ=0 (Coulomb potential), this reproduces the Rutherford scattering formula.
12.3 Resonance Scattering
When the scattering energy is near a quasi-bound state, the phase shift passes through π/2 (resonance):
δl(E)≈δbg+arctan(ER−EΓ/2)
Where ER is the resonance energy and Γ is the width. The cross section has the Breit—Wigner form:
σl(E)=k24π(2l+1)(E−ER)2+(Γ/2)2(Γ/2)2
At resonance (E=ER): σlmax=k24π(2l+1) (unitarity limit).
Worked Example 12.1: Low-Energy Scattering and Scattering Length
For s-wave scattering (l=0) at low energy (ka≪1), only the l=0 phase shift contributes:
σ≈k24πsin2δ0≈4πas2
Where the scattering lengthas is defined by kcotδ0→−1/as as k→0.
For a hard sphere of radius a: δ0=−ka (exact), giving as=a and σ=4πa2 (four times the geometric cross section πa2 --- a purely quantum result).
For the 3He—4He system: as≈1.4 nm (positive, indicating a repulsive effective potential). For the neutron—proton system (triplet): as≈5.4 fm (positive, with a bound state --- the deuteron). For singlet: as≈−23.7 fm (negative, indicating a virtual state).
Worked Example 12.2: Born Approximation for a Gaussian Potential
At low energy (ka≪1): f≈−ℏ2mV0(2π)1/2a3 (independent of θ), giving:
σ≈4π(ℏ2mV0)22πa6=ℏ48π2m2V02a6
The Born approximation is valid when ∣V0∣≪ℏ2/(ma2)I.e., the potential is weak compared to the kinetic energy associated with the length scale a.
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:Etrial≥E0 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 ρ(Ef) 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 m∣V0∣a/ℏ2≪1 where a 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 Γ. The scattering length can be much larger than the range of the potential near a resonance (the unitarity limit).
Problems (Additional)
Problem 19: Exchange Energy in Lithium
Lithium (Z=3) has the electron configuration 1s22s1. Using the variational method with Zeff for the 1s electrons:
(a) Calculate Zeff for the 1s electrons, treating the 2s electron as a perturbation.
(b) Calculate the ionisation energy (removing the 2s electron) and compare with the experimental value of 5.39 eV.
(c) Explain why the 2s electron is effectively screened by Zeff≈1.26.
Solution:
(a) For the 1s electrons, the effective charge is reduced from Z=3 by screening from the other 1s electron and partial penetration of the 2s electron. The 1s electrons screen each other partially: using the helium result, Zeff(1s)≈Z−5/16=3−0.3125=2.69.
(b) The 2s electron sees an effective nuclear charge of Zeff(2s)≈3−2×0.85=1.3 (Slater’s rules). The energy:
The ionisation energy is ∣E2s∣=5.75 eV, close to the experimental 5.39 eV. The discrepancy reflects the crudeness of the Slater screening constants.
(c) The 2s electron has significant radial extent beyond the 1s core, so it sees a nearly bare nuclear charge at small r but is screened by both 1s electrons at large r. The effective charge Zeff≈1.26 (using Hartree—Fock) represents this average screening.
Problem 20: Partial Wave Analysis for Square Well
Consider scattering from the attractive square well V(r)=−V0 for r<a and V(r)=0 for r>a.
(a) Show that the s-wave phase shift satisfies:
δ0=−ka+arctan(κktan(κa))
Where κ=2m(V0+E)/ℏ and k=2mE/ℏ.
(b) Show that a bound state exists at energy E=−∣E∣ when κ0a=π/2 where κ0=2m(V0−∣E∣)/ℏ.
(c) Show that the scattering length diverges as a new bound state appears.
Solution:
(a) Inside the well (r<a), the radial wavefunction for l=0 is u(r)=Asin(κr). Outside (r>a), u(r)=Bsin(kr+δ0).
Matching u and u′ at r=a:
κcos(κa)=kcos(ka+δ0)/sin(ka+δ0)⋅k
Wait: κcot(κa)=kcot(ka+δ0).
cot(ka+δ0)=kκcot(κa)
ka+δ0=\arccot(kκcot(κa))=arctan(κktan(κa))
δ0=−ka+arctan(κktan(κa))
(b) A bound state has E<0So k=iκ′ where κ′=2m∣E∣/ℏ. The bound state condition is that the exterior solution decays exponentially: u(r)=Be−κ′r. Matching:
κcot(κa)=−κ′
As ∣E∣→0: κ′→0So κcot(κa)→0Giving κa=π/2 (the threshold for the first bound state).
(c) The scattering length as=−limk→0(δ0/k). As κa→π/2, tan(κa)→∞So:
δ0≈−ka+arctan(∞)=−ka+π/2
as=−k1(−ka+2π)=a−2kπ
As k→0: as→±∞ (diverges), changing sign as the bound state appears.