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Gaussian Potential in the Born Approximation

This worked example computes the first Born scattering amplitude and cross section for a three-dimensional Gaussian potential

V(r)=V0e−r2/a2.V(r) = V_0e^{-r^2/a^2}.

The sign of V0V_0 determines whether the potential is repulsive or attractive, but the leading Born differential cross section depends on V02V_0^2.

Use the first Born approximation because the potential is smooth, short-ranged, and has an elementary Fourier transform.

With the scattering-amplitude convention used in this volume,

fB(q)=−m2πℏ2∫d3r e−iq⋅rV(r),f_{\mathrm B}(\mathbf q) = - \frac{m}{2\pi\hbar^2} \int d^3r\, e^{-i\mathbf q\cdot\mathbf r} V(r),

where

q=k′−k,q=2ksin⁡θ2\mathbf q=\mathbf k'-\mathbf k, \qquad q=2k\sin\frac{\theta}{2}

for elastic scattering.

The basic weak-scattering parameter is of order

ϵ∼m∣V0∣a2ℏ2.\epsilon \sim \frac{m|V_0|a^2}{\hbar^2}.

The Born result should be checked against unitarity and, when possible, numerical phase shifts as ϵ\epsilon grows.

Born Approximation Numerical Test performs that check for the repulsive Gaussian, with independent coupling, momentum, grid, matching-radius, and partial-wave sweeps.

The Gaussian integral in three dimensions is

∫d3r e−iq⋅re−r2/a2=π3/2a3e−q2a2/4.\int d^3r\, e^{-i\mathbf q\cdot\mathbf r} e^{-r^2/a^2} = \pi^{3/2}a^3 e^{-q^2a^2/4}.

Thus

∫d3r e−iq⋅rV0e−r2/a2=V0π3/2a3e−q2a2/4.\int d^3r\, e^{-i\mathbf q\cdot\mathbf r} V_0e^{-r^2/a^2} = V_0\pi^{3/2}a^3 e^{-q^2a^2/4}.

Substituting into the Born formula gives

fB(q)=−mV0π a32ℏ2e−q2a2/4.f_{\mathrm B}(q) = - \frac{mV_0\sqrt\pi\,a^3}{2\hbar^2} e^{-q^2a^2/4}.

It is useful to define

A=mV0π a32ℏ2.A = \frac{mV_0\sqrt\pi\,a^3}{2\hbar^2}.

Then

fB(q)=−Ae−q2a2/4.f_{\mathrm B}(q) = - A e^{-q^2a^2/4}.

For a real potential, the leading Born amplitude is real. Unitarity effects in the imaginary forward amplitude appear at higher Born orders.

The differential cross section is

dσdΩ=∣fB(q)∣2=A2e−q2a2/2.\frac{d\sigma}{d\Omega} = |f_{\mathrm B}(q)|^2 = A^2e^{-q^2a^2/2}.

Using

q=2ksin⁡θ2,q=2k\sin\frac{\theta}{2},

this becomes

dσdΩ=m2V02πa64ℏ4exp⁡[−2k2a2sin⁡2θ2].\frac{d\sigma}{d\Omega} = \frac{m^2V_0^2\pi a^6}{4\hbar^4} \exp \left[ - 2k^2a^2 \sin^2\frac{\theta}{2} \right].

Large-angle scattering is exponentially suppressed when kaka is large because large angles require large momentum transfer.

Let

β=k2a2.\beta=k^2a^2.

Since

q2a2/2=β(1−cos⁡θ),q^2a^2/2 = \beta(1-\cos\theta),

the total Born cross section is

σB=2πA2∫−11dμ e−β(1−μ).\sigma_{\mathrm B} = 2\pi A^2 \int_{-1}^{1} d\mu\, e^{-\beta(1-\mu)}.

Evaluating the integral,

σB=2πA21−e−2ββ.\sigma_{\mathrm B} = 2\pi A^2 \frac{1-e^{-2\beta}}{\beta}.

Restoring AA,

σB=π2m2V02a62ℏ41−e−2k2a2k2a2.\sigma_{\mathrm B} = \frac{\pi^2m^2V_0^2a^6}{2\hbar^4} \frac{1-e^{-2k^2a^2}}{k^2a^2}.

In the low-energy limit ka≪1ka\ll1,

σB→4πA2=π2m2V02a6ℏ4.\sigma_{\mathrm B} \to 4\pi A^2 = \frac{\pi^2m^2V_0^2a^6}{\hbar^4}.

The Born approximation is most reliable when the potential is weak enough that the scattered wave remains small inside the interaction region. The dimensionless estimate

ϵ∼m∣V0∣a2ℏ2\epsilon \sim \frac{m|V_0|a^2}{\hbar^2}

should be small.

At low energy, an attractive Gaussian can support or nearly support a shallow bound state as ∣V0∣|V_0| grows. Near such a threshold, the scattering length can become large and the first Born approximation fails even if the potential looks smooth.

At high energy, the angular distribution narrows because the Fourier transform suppresses momentum transfers q≳1/aq\gtrsim1/a.

At zero momentum transfer,

fB(0)=−m2πℏ2∫d3r V(r),f_{\mathrm B}(0) = - \frac{m}{2\pi\hbar^2} \int d^3r\,V(r),

so the forward amplitude is proportional to the volume integral of the potential. The Gaussian result satisfies this immediately.

The amplitude has dimensions of length:

[mV0a3ℏ2]=length.\left[ \frac{mV_0a^3}{\hbar^2} \right] = \text{length}.

The cross section depends on V02V_0^2, so the leading Born differential cross section does not distinguish attraction from repulsion. Phase shifts and higher orders do.

  • Forgetting the factor q=2ksin⁡(θ/2)q=2k\sin(\theta/2).
  • Squaring the amplitude but forgetting to double the Gaussian exponent.
  • Treating the leading real Born amplitude as if it already satisfied the optical theorem.
  • Assuming the Born approximation is reliable for any smooth potential.
  • Ignoring possible low-energy enhancement from a shallow bound state.
  • 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.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  1. Show that the low-energy total Born cross section is 4πA24\pi A^2.
Solution

For ka≪1ka\ll1,

e−q2a2/2≈1.e^{-q^2a^2/2}\approx1.

The differential cross section is approximately isotropic:

dσdΩ≈A2.\frac{d\sigma}{d\Omega}\approx A^2.

Integrating over solid angle gives

σ≈4πA2.\sigma\approx4\pi A^2.
  1. Why does the leading Born differential cross section not depend on the sign of V0V_0?
Solution

The Born amplitude is proportional to V0V_0:

fB∝V0.f_{\mathrm B}\propto V_0.

The differential cross section is the magnitude squared:

dσdΩ=∣fB∣2.\frac{d\sigma}{d\Omega}=|f_{\mathrm B}|^2.

Therefore the leading cross section is proportional to V02V_0^2 and is insensitive to the sign. The sign affects phases, higher-order terms, and possible bound-state physics.