Math 2.0

Optics, electromagnetic theory Scattering Theorem

Optical theorem

Builds on Electromagnetic scatteringHelmholtz equationPlane waveBorn approximation

Statement

Let k>0k > 0 be a wavenumber and let d^\hat{d} be a unit vector in ℝ3\R^3. Consider a time-harmonic scalar wave with time factor e−iωte^{-i\omega t} that solves the Helmholtz equation Δu+k2u=0\Delta u + k^2 u = 0 outside a bounded scatterer. Suppose the total field is u=ui+usu = u_i + u_s, where ui(x)=eikd^⋅xu_i(x) = e^{ik \hat{d} \cdot x} is the incident plane wave. Suppose the scattered field usu_s has the far-field form us(x)=f(x^)eikrr+o ⁣(1r),r=∣x∣→∞,x^=x/r,u_s(x) = f(\hat{x}) \frac{e^{ikr}}{r} + o\!\left(\frac{1}{r}\right), \qquad r = \abs{x} \to \infty, \quad \hat{x} = x / r, where ff is the scattering amplitude. Let σext\sigma_{\mathrm{ext}} be the extinction cross-section. It is the rate at which scattering and absorption take energy from the incident wave, divided by the incident energy flux per unit area. Then σext=4πkIm⁡f(d^).\sigma_{\mathrm{ext}} = \frac{4\pi}{k} \operatorname{Im} f(\hat{d}). If the scatterer does not absorb, σext\sigma_{\mathrm{ext}} equals the total scattering cross-section ∫S2∣f(x^)∣2 dΩ(x^)\int_{S^2} \abs{f(\hat{x})}^2 \, d\Omega(\hat{x}).

Remarks

The proof is a balance of energy flux through a large sphere around the scatterer. The flux of the total field splits into the flux of uiu_i, which is zero, the flux of usu_s, and a cross term between uiu_i and usu_s. For large rr, the cross term is an oscillatory integral over the sphere, and the method of stationary phase shows that only the forward direction x^=d^\hat{x} = \hat{d} contributes. This gives the term 4πkIm⁡f(d^)\frac{4\pi}{k} \operatorname{Im} f(\hat{d}).

The same identity holds for electromagnetic scattering, with the vector forward amplitude projected on the incident polarization. It also holds in quantum potential scattering, where it is a consequence of the unitarity of the scattering operator.

An example is the extinction paradox. For a large opaque sphere of radius aa with ka→∞ka \to \infty, the extinction cross-section tends to 2πa22\pi a^2, twice the geometric cross-section. Half of it comes from the light that hits the sphere, and the other half from the light diffracted into a narrow forward cone.

Going deeper

For a student

The theorem links the far-field pattern ff to the total cross-section, so it is a check on any numerical scattering code. In quantum mechanics it reads σtot=4πkIm⁡f(0)\sigma_{\mathrm{tot}} = \frac{4\pi}{k} \operatorname{Im} f(0) and follows from conservation of probability. It also constrains approximations: the Born approximation gives a real forward amplitude for a real potential, so it violates the optical theorem at first order.

Reading path

To understand this page from the ground up, read these 5 pages in order. The foundations come first.

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Each page uses the pages above it. The colour of the bar on a box shows how strong the evidence is, and the box also gives it as text. The list has the same pages.
  • no evidence level
  1. Born approximation concept
  2. Electromagnetic scattering concept
  3. Helmholtz equation concept
  4. Plane wave concept
  5. Optical theorem statement

Further reading

  1. Web https://en.wikipedia.org/wiki/Optical_theorem
About this page
TagZJG1YAGANG
URIm2://ZJG1YAGANG
Kindstatement, theorem
WritingW0 stub
MSC78A45, 35P25, 81U05
StatusThis copy of the site has no build data. Run m2 status ZJG1YAGANG.
AboutElectromagnetic scattering
UsesElectromagnetic scattering, Helmholtz equation, Plane wave, Born approximation
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Changed3 November 2026

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