Thomson Scattering Cross Section
Also known as: Classical Electron Scattering · σ_T
An EM wave shakes a free electron, which re-radiates a dipole pattern; the total scattering rate corresponds to an effective area σ_T set by the classical electron radius r_e.
Photon scatters off electron isotropically; ring pulse for σ_T.
Equivalent forms
A purely classical result that survives as the low-energy limit of QED's Compton formula.
Unit systems
Where it holds
Dimensional analysis
Thomson derived the cross section while modeling the scattering of X-rays by atomic electrons, providing one of the first quantitative tests of electron count in atoms.
How effectively does a free electron scatter low-energy light?
Compute the classical Thomson cross section using e, m_e, c, ε₀ and compare with the high-energy Klein-Nishina limit.
- Compton Gamma-Ray Observatory and X-ray polarimetry
- Solar corona electron density mapping (K-corona is Thomson-scattered photospheric light)
- Plasma diagnostics in fusion devices (laser Thomson scattering)
- Cosmic Microwave Background polarization from electron scattering
- does not depend on photon frequency — a striking classical result.
- Only valid in the long-wavelength limit; energies recoil and spin effects matter.
- Bound electrons scatter coherently with the atom (Rayleigh scattering), not as free electrons.
Limiting cases
What if…
scales as — the muon cross section is .
— would grow , making the universe even more opaque to early radiation.
Klein-Nishina suppresses ; the simple Thomson formula overestimates scattering.
Compute σ_T from constants
- e:
- 1.602176634e-19
- m e:
- 9.1093837015e-31
- c:
- 299792458
- Step 1: .
- Step 2: .
- Step 3: barn.
Mean free path of CMB photons before recombination
- σ T:
- 6.6524e-29
- Step 1: .
- Step 2: .
- Step 3: — short on cosmological scales, hence the universe was opaque.