Math 2.0

Optics, electromagnetic theory Definition

Electromagnetic scattering

Builds on Maxwell's equationsPlane waveSilver–Müller radiation conditionPermittivity

Definition

Fix an angular frequency ω>0\omega > 0 and the time factor e−iωte^{-i\omega t}, and let the background be vacuum with wavenumber k=ω/ck = \omega/c. Let the scatterer be one of two kinds. It is either a bounded obstacle D⊂ℝ3D \subset \R^3 with perfectly conducting boundary, or a medium with permittivity ε(𝐱)\varepsilon(\mathbf{x}) equal to ε0\varepsilon_0 outside a bounded set DD. Let the incident field 𝐄inc\mathbf{E}^{\mathrm{inc}} be a solution of the source-free Maxwell's equations in vacuum on all of ℝ3\R^3, such as a plane wave. The electromagnetic scattering problem is to find the total field 𝐄=𝐄inc+𝐄sc\mathbf{E} = \mathbf{E}^{\mathrm{inc}} + \mathbf{E}^{\mathrm{sc}} such that:

  1. 𝐄\mathbf{E} satisfies the time-harmonic Maxwell equations with the scatterer, outside DD for an obstacle or in all of ℝ3\R^3 for a medium;
  2. for an obstacle, 𝐧^×𝐄=0\hat{\mathbf{n}} \times \mathbf{E} = 0 on ∂D\partial D;
  3. the scattered field 𝐄sc\mathbf{E}^{\mathrm{sc}} satisfies the Silver–Müller radiation condition.

Remarks

The scattered field has the asymptotic form 𝐄sc(r𝐱^)=eikrr(𝐄∞(𝐱^)+O(1/r))\mathbf{E}^{\mathrm{sc}}(r\hat{\mathbf{x}}) = \dfrac{e^{ikr}}{r}\left( \mathbf{E}_\infty(\hat{\mathbf{x}}) + O(1/r) \right), and 𝐄∞\mathbf{E}_\infty is the far-field pattern. For an incident plane wave of unit amplitude, the scattering cross-section is Csca=∫S2∣𝐄∞∣2 dΩC_{\mathrm{sca}} = \int_{S^2} \abs{\mathbf{E}_\infty}^2 \, d\Omega, the scattered power divided by the incident intensity. The radiation condition singles out outgoing waves and makes the problem uniquely solvable for a perfect conductor. It does the same for a medium whose permittivity has non-negative imaginary part, under mild regularity assumptions. Example: a small dielectric sphere in a plane wave gives Rayleigh scattering, whose far-field pattern is that of an oscillating dipole. Non-example: the field 𝐄inc\mathbf{E}^{\mathrm{inc}} itself is not a scattered field, since a plane wave does not satisfy the radiation condition. The optical theorem relates the total power removed from the incident wave to the forward value of 𝐄∞\mathbf{E}_\infty.

Reading path

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

Show the path as a graph
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. Maxwell's equations concept
  2. Permittivity concept
  3. Plane wave concept
  4. Silver–Müller radiation condition concept
  5. Electromagnetic scattering definition

Where this leads

2 pages build on this one.

Further reading

  1. Web https://en.wikipedia.org/wiki/Scattering
About this page
TagSW593EA0A2
URIm2://SW593EA0A2
Kinddefinition
WritingW0 stub
MSC78A45, 35P25
DefinesElectromagnetic scattering
UsesMaxwell's equations, Plane wave, Silver–Müller radiation condition, Permittivity
Changed3 November 2026

Markdown · JSON · Edit on GitHub

What this page needs for W1

  • an inventory row: the row of the inventory that the node accounts for (0 of 1)
  • a source with a locator (0 of 1)

The writing levels say how complete the text of a page is. They do not measure its truth.

What links here

Used by