Skip to content

Coulomb Scattering

Coulomb scattering is the central example of long-range scattering. The potential

V(r)=κrV(r)=\frac{\kappa}{r}

falls too slowly for the standard short-range asymptotic form to apply without modification. The differential cross section has the Rutherford form, but the scattering state carries long-range logarithmic phase structure.

This page treats nonrelativistic two-body Coulomb scattering in the center-of-mass frame, with reduced mass μ\mu and relative momentum ℏk\hbar k. For the place of positive-energy states in the Coulomb spectrum before scattering amplitudes are introduced, see Continuum States of the Coulomb Problem.

For a short-range potential, the large-distance scattering state has the schematic form

ψ(r)∼eikz+f(θ)eikrr.\psi(\mathbf r) \sim e^{ikz} + f(\theta) \frac{e^{ikr}}{r}.

The Coulomb potential does not become negligible fast enough for the incident wave to remain a simple plane wave at large distance. Instead, both incoming and outgoing waves acquire Coulomb phases. This affects:

  • the definition of asymptotic states,
  • the partial-wave phase shifts,
  • the forward-angle behavior,
  • the total cross section,
  • the use of the optical theorem.

The familiar Rutherford cross section is correct, but it sits inside a more subtle scattering theory than short-range potential scattering.

Define the dimensionless Coulomb parameter

η=μκℏ2k.\eta = \frac{\mu\kappa}{\hbar^2k}.

Repulsive Coulomb scattering has κ>0\kappa>0, while attractive Coulomb scattering has κ<0\kappa<0. The energy is

E=ℏ2k22μ.E = \frac{\hbar^2k^2}{2\mu}.

The magnitude ∣η∣\lvert\eta\rvert grows at low energy, so Coulomb scattering is not a small low-energy perturbation.

The exact Coulomb differential cross section is

dσdΩ=η24k2sin⁡4(θ/2).\frac{d\sigma}{d\Omega} = \frac{\eta^2}{4k^2\sin^4(\theta/2)}.

Equivalently,

dσdΩ=κ216E2sin⁡4(θ/2).\frac{d\sigma}{d\Omega} = \frac{\kappa^2}{16E^2\sin^4(\theta/2)}.

This is the Rutherford formula. It agrees with the classical result for a 1/r1/r force.

The forward divergence as θ→0\theta\to0 reflects the long range of the force. The total cross section obtained by integrating over all angles diverges unless screening, finite beam geometry, or an angular cutoff is included.

One common convention for the Coulomb amplitude is

fC(θ)=−η2ksin⁡2(θ/2)exp⁡[2iσ0−2iηln⁡sin⁡θ2],f_C(\theta) = - \frac{\eta}{2k\sin^2(\theta/2)} \exp \left[ 2i\sigma_0 - 2i\eta\ln\sin\frac{\theta}{2} \right],

where

σℓ=arg⁡Γ(ℓ+1+iη)\sigma_\ell = \arg\Gamma(\ell+1+i\eta)

is the Coulomb phase shift. The phase convention may differ between texts, but the magnitude gives the Rutherford cross section:

∣fC(θ)∣2=η24k2sin⁡4(θ/2).\lvert f_C(\theta)\rvert^2 = \frac{\eta^2}{4k^2\sin^4(\theta/2)}.

The logarithm in the phase is a signature of the long-range tail. It has no analogue for ordinary finite-range potentials.

For Coulomb scattering, the partial-wave SS-matrix contains Coulomb phases

SℓC=e2iσℓ.S_\ell^{C} = e^{2i\sigma_\ell}.

Unlike short-range scattering, infinitely many partial waves contribute significantly because the interaction reaches arbitrarily large impact parameters.

When a short-range nuclear or atomic potential is added to a Coulomb interaction, one often separates the known Coulomb phases from additional short-range phase shifts:

Sℓ=e2iσℓe2iδℓshort.S_\ell = e^{2i\sigma_\ell} e^{2i\delta_\ell^{\mathrm{short}}}.

This separation is essential in charged-particle scattering.

Formally, the Fourier transform of the Coulomb potential is

∫d3r e−iq⋅rκr=4πκq2.\int d^3r\, e^{-i\mathbf q\cdot\mathbf r} \frac{\kappa}{r} = \frac{4\pi\kappa}{q^2}.

Substituting this into the first Born formula gives

fB(q)=−2μκℏ2q2.f_{\mathrm B}(q) = - \frac{2\mu\kappa}{\hbar^2q^2}.

For elastic scattering,

q=2ksin⁡θ2,q=2k\sin\frac{\theta}{2},

so

∣fB∣2=η24k2sin⁡4(θ/2).\lvert f_{\mathrm B}\rvert^2 = \frac{\eta^2}{4k^2\sin^4(\theta/2)}.

The magnitude matches the Rutherford cross section. This agreement is special. It does not mean the unscreened Coulomb problem is a well-behaved ordinary Born approximation: the exact phase and asymptotic states are long-range modified, and the forward divergence remains. Validity of the Born Approximation explains why magnitude agreement does not establish convergence and compares short-range and Coulomb diagnostics.

Real scattering experiments rarely involve an ideal infinite Coulomb field with perfect angular resolution. Atomic electrons screen nuclear charge at long distances. Beams have finite size. Detectors exclude a small forward cone. Plasmas have Debye screening.

A screened Coulomb potential behaves like a short-range potential beyond the screening length. One may compute with screening and then take controlled limits for observables that remain finite. Inclusive or cutoff-defined observables are often more physical than a formal total cross section.

Yukawa Potential in the Born Approximation performs this calculation explicitly and shows that removing the screening makes the total cross section diverge as the inverse screening scale squared while the momentum-transfer cross section diverges only logarithmically.

Rutherford scattering provided decisive evidence for a compact atomic nucleus. The angular dependence

1sin⁡4(θ/2)\frac{1}{\sin^4(\theta/2)}

is so distinctive that large-angle scattering directly revealed strong deflections from a concentrated charge.

In modern language, the result is a bridge between classical trajectories, exact quantum Coulomb wavefunctions, and perturbative exchange amplitudes.

  • Applying short-range asymptotic formulas to the unscreened Coulomb problem without modification.
  • Expecting a finite total cross section after integrating down to θ=0\theta=0.
  • Treating the Born-result magnitude as proof that all Coulomb phases are perturbative.
  • Using ordinary low-energy scattering-length formulas for a 1/r1/r potential.
  • Forgetting the sign convention for η\eta when distinguishing attraction and repulsion.
  • E. Rutherford, “The scattering of alpha and beta particles by matter and the structure of the atom,” Philosophical Magazine 21, 669-688, 1911.
  • L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
  • A. Messiah, Quantum Mechanics, Dover, 1999.
  • J. R. Taylor, Scattering Theory: The Quantum Theory of Nonrelativistic Collisions, Dover, 2006.
  • R. G. Newton, Scattering Theory of Waves and Particles, 2nd ed., Dover, 2002.
  1. Starting from the Born amplitude
fB(q)=−2μκℏ2q2,f_{\mathrm B}(q) = - \frac{2\mu\kappa}{\hbar^2q^2},

derive the Rutherford angular dependence.

Solution

For elastic scattering,

q=2ksin⁡θ2.q=2k\sin\frac{\theta}{2}.

Therefore

fB=−2μκℏ214k2sin⁡2(θ/2)=−η2ksin⁡2(θ/2).f_{\mathrm B} = - \frac{2\mu\kappa}{\hbar^2} \frac{1}{4k^2\sin^2(\theta/2)} = - \frac{\eta}{2k\sin^2(\theta/2)}.

Taking the magnitude squared gives

dσdΩ=∣fB∣2=η24k2sin⁡4(θ/2).\frac{d\sigma}{d\Omega} = \lvert f_{\mathrm B}\rvert^2 = \frac{\eta^2}{4k^2\sin^4(\theta/2)}.
  1. Why does the total Coulomb cross section diverge?
Solution

Near θ=0\theta=0,

sin⁡θ2≈θ2,\sin\frac{\theta}{2}\approx\frac{\theta}{2},

so

dσdΩ∝1θ4.\frac{d\sigma}{d\Omega} \propto \frac{1}{\theta^4}.

The solid-angle element behaves as dΩ≈2πθ dθd\Omega\approx2\pi\theta\,d\theta, so the forward integral contains

∫θ dθθ4=∫dθθ3,\int^{ } \frac{\theta\,d\theta}{\theta^4} = \int^{ } \frac{d\theta}{\theta^3},

which diverges at the lower limit. Physical screening or angular cutoffs are needed.

  1. Explain why the agreement between the Born magnitude and the Rutherford cross section does not make Coulomb scattering an ordinary short-range Born problem.
Solution

The Coulomb potential is long-ranged, so the standard plane-wave plus outgoing spherical-wave asymptotic form is modified by Coulomb phases. The exact amplitude contains a logarithmic angular phase and Coulomb phase shifts. The Born expression reproduces the magnitude of the Rutherford cross section, but it does not reproduce the full long-range phase structure or remove the forward divergence.